AIPS version = /home/auto/aips/31DEC06/LINUX/SYSTEM/VLA_PIPE/aips Prep version = Aug 10 14:21 /home/auto/bin/AVLAPREP.001 Pipe version = Aug 10 14:21 /home/auto/bin/AVLAPIPE.001 Post version = Sep 7 11:26 /home/auto/bin/AVLAPOST.001 ------------- START_AIPS: Your initial AIPS printer is the GNU Ghostview X-windows previewer START_AIPS: - system name gv, AIPS type PREVIEW START_AIPS: User data area assignments: (Using private file /users/vlbacald/.dadevs for DADEVS.PL) Disk 1 (1) is /home/auto/aips/DATA/AUTO_1 Tape assignments: Tape 1 is REMOTE Tape 2 is REMOTE START_AIPS: Starting TPMON daemons on AUTO asynchronously... Starting up 31DEC06 AIPS with normal priority AIPS 3: You are NOT assigned a TV device or server AIPS 3: You are NOT assigned a graphics device or server AIPS 3: Enter user ID number ?AIPS 3: 31DEC06 AIPS: AIPS 3: Copyright (C) 1995-2006 Associated Universities, Inc. AIPS 3: AIPS comes with ABSOLUTELY NO WARRANTY; AIPS 3: for details, type HELP GNUGPL AIPS 3: This is free software, and you are welcome to redistribute it AIPS 3: under certain conditions; type EXPLAIN GNUGPL for details. AIPS 3: Previous session command-line history recovered. AIPS 3: TAB-key completions enabled, type HELP READLINE for details. AIPS 3: Recovered POPS environment from last exit >>>AIPS 3: Found in Version=ABIN AIPS 3: $ Lorant Sjouwerman, versions 1.. 2005, for NRAO AIPS 3: AIPS 3: $$ General naming utilities - default to data disk 1 (safest of all) AIPS 3: procedure pipedef1 AIPS 3: string*12 pnam AIPS 3: string*6 pcls AIPS 3: scalar pseq,pdsk AIPS 3: pdsk=1 AIPS 3: finish AIPS 3: pipedef1 AIPS 3: procedure namepipe AIPS 3: pnam=inname;pcls=inclass;pseq=inseq;indisk=pdsk AIPS 3: finish AIPS 3: procedure pipename AIPS 3: inname=pnam;inclass=pcls;inseq=pseq;indisk=pdsk AIPS 3: finish AIPS 3: AIPS 3: procedure checkcat AIPS 3: $LOS - count and make sure catalog starts at one (and not more t han 10 files) AIPS 3: scalar numcat AIPS 3: clrname;indisk=pdsk;chkname;numcat=1-error AIPS 3: $ for later: find out how to deal with CH0/LINE data in MOVE AIPS 3: if(numcat>0)then;recat;end;clrtemp AIPS 3: return numcat AIPS 3: finish AIPS 3: AIPS 3: procedure gx AIPS 3: $ inputs AIPS 3: go;wait AIPS 3: finish AIPS 3: AIPS 3: procedure pre_fillm AIPS 3: $LOS - sets VLA archive defaults for fillm AIPS 3: default fillm;outdisk=pdsk;doall=1;douvcomp=-1;cparm(8)=0.05;b parm(10)=0.75 AIPS 3: finish AIPS 3: AIPS 3: procedure fname AIPS 3: return inname!!'.'!!inclass!!'.'!!char(inseq) AIPS 3: finish AIPS 3: AIPS 3: procedure del AIPS 3: error=1;zap AIPS 3: finish AIPS 3: AIPS 3: procedure skipdata AIPS 3: $LOS - delete unwanted data sets - currently all but continuum X and C bands AIPS 3: $ if(inclass='LINE')then;del;inclass'CH 0';del;type'ZAP LINE :' fname;end AIPS 3: if((inclass='CH 0')!(inclass='LINE'))then;del;type'ZAP LINE :' fname;end AIPS 3: if(inclass='4 BAND')then;del;type'ZAP 4-BAND :'fname;end AIPS 3: if(inclass='P BAND')then;del;type'ZAP P-BAND :'fname;end AIPS 3: if(inclass='L BAND')then;del;type'ZAP L-BAND :'fname;end AIPS 3: if(inclass='U BAND')then;del;type'ZAP U-BAND :'fname;end AIPS 3: if(inclass='K BAND')then;del;type'ZAP K-BAND :'fname;end AIPS 3: if(inclass='Q BAND')then;del;type'ZAP Q-BAND :'fname;end;clrte mp AIPS 3: if(error<1)then $ file not zapped, check for single dish vlbi; #vis=0 AIPS 3: task'TABGET';userid 0;inext'NX';invers=0;keyvalue=0;keystrng '' AIPS 3: keyword'NUM ROW';getthead;pixxy=keyvalue(1),6,0;tabget;clrte mp AIPS 3: if(keyvalue(1)=0)then;del;type'ZAP S-DISH :'fname;end AIPS 3: end AIPS 3: $also zap if solar/planetary/pulsar mode - su table proper motio n?? AIPS 3: $ and what about PT-link? antenna VPT is not OUT, later also EV LA names AIPS 3: finish AIPS 3: AIPS 3: procedure checkids AIPS 3: $LOS - account for fast switching source names - check on pos, q ual, calco AIPS 3: scalar ra1a,ra1b,ra2a,ra2b,dc1a,dc1b,dc2a,dc2b,n,m,l,idx AIPS 3: scalar q1,q2 AIPS 3: string*1 co1,co2 AIPS 3: string*16 n1,n2 AIPS 3: array alist(100),blist(100) AIPS 3: inext'SU';invers 0;keyword'NUM ROW';keyvalue 0;keystrng'';gett head AIPS 3: n=keyvalue(1);idx=1;aparm 0;bparm 0;alist 0;blist 0 AIPS 3: if (n > 1) then AIPS 3: for m=1:(n-1);clrtemp AIPS 3: pixxy m,11;tabget;ra1a keyvalue(1);ra1b keyvalue(2) AIPS 3: for l=(m+1):n;clrtemp AIPS 3: pixxy l,11;tabget;ra2a keyvalue(1);ra2b keyvalue(2) AIPS 3: if (abs(ra1a-ra2a)=0) then AIPS 3: if ( abs((ra1b-ra2b)*3600*1000) < 3 ) then $ RA within 3 mas! AIPS 3: pixxy m,12;tabget;dc1a keyvalue(1);dc1b keyvalue(2) AIPS 3: pixxy l,12;tabget;dc2a keyvalue(1);dc2b keyvalue(2) AIPS 3: if (abs(dc1a-dc2a)=0) then AIPS 3: if ( abs((dc1b-dc2b)*3600*1000) < 3 ) then $ DC wi thin 3 mas! AIPS 3: pixxy m,3;tabget;q1 keyvalue(1);pixxy l,3;tabget ;q2 keyvalue(1) AIPS 3: if (q1=q2) then $ same qualifier; same calcode? AIPS 3: pixxy m,4;tabget;co1 keystrng;pixxy l,4;tabget ;co2 keystrng AIPS 3: if (co1=co2) then AIPS 3: pixxy m,1;tabget;q1 keyvalue(1) AIPS 3: pixxy l,1;tabget;q2 keyvalue(1) AIPS 3: pixxy m,2;tabget;n1 keystrng;pixxy l,2;tabge t;n2 keystrng AIPS 3: if (idx>100) then; AIPS 3: type 'TOO MANY SOURCES TO DO DSORC - DO BY HAND!' AIPS 3: type 'NEXT =.'!!char(idx)!!' DO:'!!char(l)! !'.&.'!!char(m) AIPS 3: else AIPS 3: if (length(n1)1) then;task'DSORC';n=0 AIPS 3: outname inname;outclass inclass;outseq inseq;outdisk indis k AIPS 3: while (n100)then;type'TOO MANY SOURCES FOR DSORC';error 1;end ;clrtemp AIPS 3: end AIPS 3: finish AIPS 3: AIPS 3: procedure checkcal AIPS 3: $LOS Currently (Sep 22, 2005) can/will do 3C286 and 3C48 at X and C AIPS 3: $LOS (and for now skip 3C286/3C48/3C138/3C147 Q,K,U and 3C48 L ) AIPS 3: scalar idx,jdx AIPS 3: string*16 sname AIPS 3: task'TABGET';userid 0;inext'SU';invers=0;keyvalue=0;keystrng'' ;error=1 AIPS 3: keyword'NUM ROW';getthead;idx=keyvalue(1);clrtemp AIPS 3: for jdx=1:idx AIPS 3: pixxy=jdx,2,0;tabget;sname=substr(keystrng,1,length(keystrng )) AIPS 3: if(sname='3C286')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='3C48')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='3C138')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='3C147')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='3C295')then;error=-1;jdx=idx+1;end AIPS 3: if(error>0)then $ try B1950 name AIPS 3: if(sname='1328+307')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='0134+329')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='0518+165')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='0538+498')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='1409+524')then;error=-1;jdx=idx+1;end AIPS 3: if(error>0)then $ try J2000 AIPS 3: if(sname='1331+305')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='0137+331')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='0521+166')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='0542+498')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='1411+522')then;error=-1;jdx=idx+1;end AIPS 3: if(error>0)then $ try J2000 name AIPS 3: if(sname='J1331+3030')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='J0137+3309')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='J0521+1638')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='J0542+4951')then;error=-1;jdx=idx+1;end AIPS 3: if(sname='J1411+5212')then;error=-1;jdx=idx+1;end AIPS 3: end;end;end;clrtemp AIPS 3: end AIPS 3: $ if error>0 check on coords (for different name than standard) AIPS 3: $ but keyval not reliable to do this.. ?? AIPS 3: $ end AIPS 3: if(error>0)then;del;type'ZAP - NO STD CAL SRC FOR :'fname;erro r=1 AIPS 3: else;checkids;error=-1;end;clrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure j2000fix AIPS 3: $LOS - convert data to J2000 by default use of uvfix AIPS 3: task'UVFIX';outname=inname;outclass=inclass;outseq=inseq;outdi sk=indisk AIPS 3: shift=0;uvfixprm=0;tput uvfix;outclass'PREFIX';rename AIPS 3: tget uvfix;inclass'PREFIX';gx;zap;inclass=outclass;clrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure datachks AIPS 3: $LOS - delete unwanted data sets, check for standard calibrators and make J2000 AIPS 3: if(error<1)then $ file exists AIPS 3: skipdata;if(error<1)then $ file was not zapped AIPS 3: checkcal;if(error<1)then $ file has standard calibrator i n it AIPS 3: j2000fix AIPS 3: $ addcalco AIPS 3: end;end;end;clrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure freqchks AIPS 3: $LOS - split up in frequency IDs, run INDXR, and remove AIPS 3: scalar rows, nfrq AIPS 3: if(error<1)then $ file exists AIPS 3: inext'FQ';invers=1;keyword='NUM ROW';getthead;nfrq=keyvalue( 1) AIPS 3: if (nfrq > 1) then AIPS 3: if (nfrq > 9) then;type' WARNING! MORE THAN 9 FREQUENCY ID -S!';end AIPS 3: tput getthead;default'UVCOP';tget getthead;keyword='';task 'UVCOP';tput AIPS 3: for rows=1:nfrq AIPS 3: pixxy=rows,1,1;inver=1;inext='FQ';tabget;tget;freqid=key value(1) AIPS 3: outclass=substr(inclass,1,1)!!substr(inclass,3,6)!!char( freqid) AIPS 3: type'COPYING FREQUENCY ID #'!!char(freqid);gx AIPS 3: default'INDXR';tget uvcop;task'INDXR';inclass outclass;g x;task'DQUAL' AIPS 3: $out not in! ** outname=inname;outclass=inclass;outseq=inseq;out disk=indisk;gx AIPS 3: tget uvcop;freqid=1;clrtemp AIPS 3: end;end;end;if(nfrq>1)then;type fname!!' SPLIT IN :'!!char(nfr q);zap;end AIPS 3: finish AIPS 3: AIPS 3: procedure pre_move AIPS 3: $LOS - moves file to another AIPS user number AIPS 3: default move;indisk=pdsk;outseq=-1;opcode'MOVE';clrtemp AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: $ AIPS 3: $ Ver 1.0 : Copy of private Ver 3.0 of VLARUN (public version is 2.5): AIPS 3: $ was 3.0 : Add PLVER (in goplt) for plot files and to include T ASAV (12MAY04) AIPS 3: $ Repositioned inseq=0 to safeguard to SU-tab confusio n (12NOV04) AIPS 3: $ Rearanged inputs and options, added integration time calculation, AIPS 3: $ QUACK, selective plotting, INNAME vs DOCAT, alternat ive flux cal, AIPS 3: $ selective imaging, SCIMG for targets, use model in C ALIB, find VLA AIPS 3: $ array, use model,.. AIPS 3: $ AIPS 3: $Next vers add polarization calibration, SCIMG->SCIMG? AIPS 3: $ find imsize, find cutoffflux, include infi le AIPS 3: $--------------------------------------------------------------- AIPS 3: $000000001111111111222222222233333333334444444444555555555566666 6666677777777778 AIPS 3: $234567890123456789012345678901234567890123456789012345678901234 5678901234567890 AIPS 3: $=============================================== AIPS 3: $! Calibrating amplitude and phase, and imaging VLA data AIPS 3: $# RUN POPS VLA UTILITY CALIBRATION IMAGING AIPS 3: $--------------------------------------------------------------- AIPS 3: $; Copyright (C) 2002-2006 AIPS 3: $; Associated Universities, Inc. Washington DC, USA. AIPS 3: $; AIPS 3: $; This program is free software; you can redistribute it and/o r AIPS 3: $; modify it under the terms of the GNU General Public License as AIPS 3: $; published by the Free Software Foundation; either version 2 of AIPS 3: $; the License, or (at your option) any later version. AIPS 3: $; AIPS 3: $; This program is distributed in the hope that it will be usef ul, AIPS 3: $; but WITHOUT ANY WARRANTY; without even the implied warranty of AIPS 3: $; MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See th e AIPS 3: $; GNU General Public License for more details. AIPS 3: $; AIPS 3: $; You should have received a copy of the GNU General Public AIPS 3: $; License along with this program; if not, write to the Free AIPS 3: $; Software Foundation, Inc., 675 Massachusetts Ave, Cambridge, AIPS 3: $; MA 02139, USA. AIPS 3: $; AIPS 3: $; Correspondence concerning AIPS should be addressed as follow s: AIPS 3: $; Internet email: aipsmail@nrao.edu. AIPS 3: $; Postal address: AIPS Project Office AIPS 3: $; National Radio Astronomy Observatory AIPS 3: $; 520 Edgemont Road AIPS 3: $; Charlottesville, VA 22903-2475 USA AIPS 3: $--------------------------------------------------------------- AIPS 3: $=============================================================== AIPS 3: AIPS 3: procedure pipeinit AIPS 3: scalar lsdisk,lsname,lsrant,lscont,lserr,lsplot,lsflag,k,lsflu x,lstarg,lsmodl AIPS 3: scalar lsids,star,tint,fsw AIPS 3: string*2 lstyp AIPS 3: string*3 lsvla AIPS 3: string*6 lsidc,lsstrng AIPS 3: string*16 lsidn,lscal AIPS 3: string*16 lsampcal(20),lsbndcal(5),lsphacal(20),lspntcal(25),l sallcal(30), AIPS 3: array lsbadd(10),lsparm(16),lssid(1000) $ D=1,C=3.3,B=10.8,A=3 5.4,PT=73 AIPS 3: string*20 expnm AIPS 3: string*48 expmsg AIPS 3: finish AIPS 3: pipeinit AIPS 3: AIPS 3: procedure pipeinpt AIPS 3: lsampcal '3C48', '0134+329','0137+331','J0137+3309' AIPS 3: lsampcal(5)~ '3C138','0518+165','0521+166','J0521+1638' AIPS 3: lsampcal(9)~ '3C147','0538+498','0542+498','J0542+4951' AIPS 3: lsampcal(13)~'3C286','1328+307','1331+305','J1331+3030' AIPS 3: lsampcal(17)~'3C295','1409+524','1411+522','J1411+5212' AIPS 3: lserr=0;lsbadd=baddisk;lsdisk=indisk;lsname=docat AIPS 3: lsidn=inname;lsidc=inclass;lsids=inseq;lstyp'UV';fsw=doalign;l sflag=flagver AIPS 3: lsparm(2)=solint;lsparm(13)=factor;lsrant=refant;lsmodl=domode l AIPS 3: lscal=keystrng;lsflux=flux;lsparm(3)=uvrange(1);lsparm(4)=uvra nge(2) AIPS 3: for k=1:20;lsphacal(k)=sources(k);end;for k=1:5;lsbndcal(k)=ca lsour(k);end AIPS 3: lsparm(11)=dopol;lsparm(12)=bpa;lscont=docont;lsplot=plver;lsp arm(1)=doall AIPS 3: lsparm(5)=doarray;lsparm(6)=imsize(1);lsparm(7)=niter;lsparm(8 )=cutoff AIPS 3: lsparm(9)=docal;lsparm(10)=doresid AIPS 3: $ check input values AIPS 3: $->lsbadd AIPS 3: if (lsdisk<=0) then;lserr=1;type'SPECIFY THE INDISK';end AIPS 3: if(lsname<=0)then;inname=lsidn;inclass=lsidc;inseq=lsids;intyp e=lstyp;chkname AIPS 3: if (error<>0) then AIPS 3: lserr=2; type 'SPECIFY INNAME, ETC, OR THE CATALOG NUMBER = DOCAT' AIPS 3: else AIPS 3: userid=0;k=1;lsname=0 AIPS 3: while (lsname=0);egetname k AIPS 3: if (( (lsidn=inname)&(lsidc=inclass) )&(lsids=inseq)) th en AIPS 3: lsname=k;lsidn=inname;lsidc=inclass;lsids=inseq;lstyp= intype AIPS 3: else;k=k+1;end;end;end;else AIPS 3: if ( ((inname <> '')!(inclass <> '')) ! (inseq <> 0) ) then AIPS 3: lserr=2; type 'DO NOT SPECIFY BOTH INNAME, ETC, AND VARIAB LE DOCAT' AIPS 3: else AIPS 3: getname(lsname);lsidn=inname;lsidc=inclass;lsids=inseq;lst yp=intype AIPS 3: end AIPS 3: end AIPS 3: AIPS 3: $->inname AIPS 3: $->inclass AIPS 3: $->inseq AIPS 3: $->fsw AIPS 3: $->lsflag AIPS 3: if (lsparm(2)<=0) then; lserr=3; type 'SPECIFY THE SOLUTION IN TERVAL';end AIPS 3: if (lsparm(13)<1)then;lsparm(13)=1;type'FACTOR<1 QUESTIONABLE, SET TO 1';end AIPS 3: if (lsrant<=0)then;lsrant=0;type'AIPS WILL CHOOSE THE REFERENC E ANTENNA';end AIPS 3: if ( (lsmodl>0) & (length(lscal)>0) ) then AIPS 3: lserr=4;type 'CANNOT USE STANDARD SOURCE MODEL FOR ALTERNATI VE CALIBRATOR' AIPS 3: end AIPS 3: $->lscal AIPS 3: if (length(lscal)<>0) then AIPS 3: type 'USING NON-STANDARD AMPLITUDE CALIBRATOR, FLUX, UVRAN GE :' AIPS 3: type lscal, lsflux, lsparm(3), lsparm(4);lsampcal='';lsamp cal(1)=lscal AIPS 3: end AIPS 3: AIPS 3: $->lsflux AIPS 3: $-> #3+#4 uvrange AIPS 3: for i=1:20;for j=1:16;if(substr(lsphacal(i),j,j)='*')then;if ( lserr<>7) then AIPS 3: if((i=1)&(j=1))then;star=1;else; AIPS 3: star=-1;lserr=7;type'ONLY USE * IN THE 1ST CHARACTER OF TH E 1ST SOURCE' AIPS 3: end;end;end;end;clrtemp;end AIPS 3: if (lsname>0) then; indisk=lsdisk; getname(lsname); clrtemp AIPS 3: if ( (inclass='CH 0') & (substr(lsbndcal(1),1,1) = ' ') ) th en AIPS 3: lserr=8;type 'SPECIFY THE BANDPASS CALIBRATOR = CALSOUR' AIPS 3: end;end;clrtemp AIPS 3: $-> #11 dopol AIPS 3: $-> #12 bpa AIPS 3: $->lscont AIPS 3: $->lsplot AIPS 3: if (lsparm(1) > 0) then AIPS 3: if (lsparm(5)<0) then;type 'SETFC WILL DETERMINE THE CELL SI ZE' AIPS 3: else; AIPS 3: if (lsparm(5)=0) then; AIPS 3: keyword='TELESCOP';gethead; AIPS 3: if (substr(keystrng,1,3)<>'VLA') then; AIPS 3: lserr=5; type 'CANNOT DETERMINE ARRAY - THIS IS NOT TH E VLA' AIPS 3: else;keyword'NUM ROW';inext'AN';invers=0;getthead;k=keyv alue(1) AIPS 3: for j=1:k AIPS 3: pixxy=j,1,0;tabget;i=1;clrtemp AIPS 3: while((substr(keystrng,i,i)<>':')&(i<9));i=i+1;end AIPS 3: if (substr(keystrng,i+1,i+1)<>' ')then; AIPS 3: lsvla=substr(keystrng,i+1,i+3);else AIPS 3: lsvla=substr(keystrng,i+2,i+4);end AIPS 3: if ((lsvla<>'OUT')&(lsvla<>'MPD'))then; AIPS 3: if (lsvla='VPT')then;lsparm(5)=75;else AIPS 3: if (substr(keystrng,i+1,i+1)<>' ')then; AIPS 3: keyword=substr(keystrng,i+2,i+8);else AIPS 3: keyword=substr(keystrng,i+3,i+9);end AIPS 3: lsparm(5)=max(lsparm(5),value(keyword));clrtem p;end;end;end AIPS 3: if (lsparm(5)<75) then;if (lsparm(5)>36) then;lsparm(5 )=36;else AIPS 3: if (lsparm(5)>18) then;lsparm(5)=11;else AIPS 3: if(lsparm(5)>9)then;lsparm(5)=3.5;else;lsparm(5)=1;end ;end;end;end AIPS 3: end;if(lsparm(5)=0)then;lserr=5;type'WHAT ARRAY?! USE DO ARRAY';else AIPS 3: if(lsparm(5)>0)then AIPS 3: type char(lsparm(5))!!' KILOMETERS WILL BE USED AS MAX IMUM BASELINE' AIPS 3: end;end;end;end AIPS 3: if (lsparm(6)>=0)then;if((lsparm(6)<128)!(imsize(2)<128))the n AIPS 3: lserr=6; type 'SPECIFY THE IMSIZE CORRECTLY (>127 OR <0)'; end;end AIPS 3: AIPS 3: $-> #7 niter AIPS 3: if (lsparm(7) < 0) then; lsparm(7) = 1e6; end AIPS 3: $-> #8 cutoff AIPS 3: $-> #9 docal AIPS 3: $-> #10 doresid AIPS 3: AIPS 3: end AIPS 3: finish AIPS 3: AIPS 3: procedure getidn AIPS 3: indisk=lsdisk;inname=lsidn;inclass=lsidc;inseq=lsids;intype=ls typ AIPS 3: finish AIPS 3: AIPS 3: procedure getset AIPS 3: default;getidn;clrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure lsclrcal AIPS 3: $ consolidate lists, deal with calcode='*' later AIPS 3: scalar lsidx,l,m,n AIPS 3: task'TABGET';getset;inext'NX';invers 0;keyvalue=0;keystrng'' AIPS 3: keyword'NUM ROW';getthead;lsidx=keyvalue(1);clrtemp;n=0;lssid= 0 AIPS 3: if (keyvalue(1)>1000)then;type'WARNING: MORE THAN 1000 SCANS ! ';end AIPS 3: for i=1:lsidx $ remember source number AIPS 3: pixxy=i,3,0;tabget;error=0 AIPS 3: for l=1:n;if(lssid(l)=keyvalue(1))then;error=1;end;end;clrte mp AIPS 3: if(error=0)then;n=n+1;lssid(n)=keyvalue(1);end AIPS 3: end;inext'SU';invers 0;keyvalue=0;keystrng'';keyword'NUM ROW' AIPS 3: getthead;lsidx=keyvalue(1);clrtemp;sources'';l=1;m=1;n=1 AIPS 3: for i=1:lsidx AIPS 3: pixxy=i,2,0;tabget;k=length(keystrng);j=0;clrtemp AIPS 3: while (j<20);j=j+1;if (substr(lsampcal(j),1,k)=substr(keystr ng,1,k)) then AIPS 3: lsampcal(l)=lsampcal(j);j=30;lsparm(14)=l;l=l+1;end;end; j=0;clrtemp AIPS 3: while (j<20);j=j+1;if (substr(lsphacal(j),1,k)=substr(keystr ng,1,k)) then AIPS 3: lsphacal(m)=lsphacal(j);j=30;lsparm(15)=m;m=m+1;end;end; j=0;clrtemp AIPS 3: while (j<5);j=j+1;if (substr(lsbndcal(j),1,k)=substr(keystrn g,1,k)) then AIPS 3: lsbndcal(n)=lsbndcal(j);j=30;lsparm(16)=n;n=n+1;end;end; clrtemp AIPS 3: end;lspntcal'';lsallcal'';for j=l:20;lsampcal(j)='';end AIPS 3: for j=m:20;lsphacal(j)='';end;for j=n:5;lsbndcal(j)='';end AIPS 3: for j=1:lsparm(15);lspntcal(j)=lsphacal(j);end;k=lsparm(15) AIPS 3: for j=1:lsparm(16);lspntcal(j+k)=lsbndcal(j);end;j=0;l=1;clrte mp AIPS 3: while (j<(lsparm(15)+lsparm(16)));j=j+1;if (length(lspntcal(j) )>0) then AIPS 3: lspntcal(l)=lspntcal(j);if(l<>j)then;lspntcal(j)='';end;l=l+ 1;end;end AIPS 3: $here - clean up pnt cal for doubles - subtract from total count below AIPS 3: k=lsparm(15)+lsparm(16);for j=1:k;lsallcal(j)=lspntcal(j);end; l=1 AIPS 3: for j=1:lsparm(14);i=length(lsampcal(j));lsidx=0;m=j AIPS 3: while ((lsidx0) then;lsallcal(l)=lsallcal(j) AIPS 3: if(l<>j)then;lsallcal(j)='';end;l=l+1;end;end AIPS 3: $typ 'LSAMPCAL, LSPHACAL, LSBNDCAL, LSPNTCAL, AND LSALLCAL :' AIPS 3: $typ lsampcal; typ lsphacal; typ lsbndcal; typ lspntcal; typ lsa llcal; AIPS 3: return;clrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure numtab(lsstrng) AIPS 3: keystrng'';j=0;clrtemp AIPS 3: while ((j<15)&(keystrng<>lsstrng)) AIPS 3: j=j+1;keyword'EXTYPE'!!char(j);gethead;end;clrtemp AIPS 3: if (keystrng=lsstrng) then AIPS 3: keyword'EXTVER'!!char(j);gethead;else;keyvalue=0;end AIPS 3: keyword'';keystrng'';clrtemp AIPS 3: return keyvalue(1);finish AIPS 3: AIPS 3: procedure numbasel AIPS 3: scalar numarow,numbout,numbant,numbase,idx;string*16 nameant AIPS 3: numbout=0;keyword'NUM ROW';inext'AN';invers=0;getthead;numarow =keyvalue(1) AIPS 3: for numbant=1:numarow AIPS 3: pixxy=numbant,1,0;tabget;nameant=keystrng;idx=1;clrtemp AIPS 3: while(substr(nameant,idx,idx)<>':');idx=idx+1;end AIPS 3: if(substr(nameant,idx+1,idx+3)='OUT')then;numbout=numbout+1; end AIPS 3: if(substr(nameant,idx+2,idx+4)='OUT')then;numbout=numbout+1; end AIPS 3: end;numbase=(numarow-numbout)*(numarow-numbout-1)/2;clrtemp AIPS 3: $ type char(numarow-numbout)!!' ANTENNAS',char(numbase)!!' BASE LINES' AIPS 3: return numbase AIPS 3: finish AIPS 3: AIPS 3: procedure calcintt AIPS 3: scalar numxrow,numscan,numbbeg,numbend,numcnst,sum,avr,rms,rma x;rmax=300 AIPS 3: array interval(1000),numbvis(1000);avr=0;if(rmax>1000)then;rma x=1000;end AIPS 3: if (numtab('NX')<1) then;type'NOT MULTISOURCE - NO INTTIME CAL CULATED' AIPS 3: else AIPS 3: keyword'NUM ROW';inext'NX';invers 0;getthead;numxrow=keyvalu e(1) AIPS 3: if(numxrow>rmax)then;numxrow rmax;end AIPS 3: for numscan=1:numxrow;clrtemp AIPS 3: pixxy=numscan,2,0;tabget;interval(numscan)=86400*keyvalue( 1) AIPS 3: pixxy=numscan,5,0;tabget;numbbeg=keyvalue(1) AIPS 3: pixxy=numscan,6,0;tabget;numbend=keyvalue(1) AIPS 3: numbvis(numscan)=numbend-numbbeg+1;avr=max(avr,numbvis(num scan)) AIPS 3: end;numcnst=numbasel;sum=0 AIPS 3: if (avr > 0) then AIPS 3: for numscan=1:numxrow;if (numbvis(numscan)>0) then AIPS 3: sum=sum+( (numcnst*interval(numscan)) / numbvis(numsca n) ) AIPS 3: end;end;clrtemp;avr=sum/numxrow;sum=0 AIPS 3: for numscan=1:numxrow;if (numbvis(numscan)>0) then AIPS 3: sum=sum+((numcnst*interval(numscan))/numbvis(numscan)- avr)**2 AIPS 3: end;end;clrtemp;rms=sum/numxrow;clrtemp;end AIPS 3: $ type char(numxrow)!!' SCANS/SAMPLES WITH RMS(SEC) +/-'!!char( rms) AIPS 3: $ type char(avr)!!' SECOND INTEGRATIONS (APPROXIMATELY)' AIPS 3: end AIPS 3: return avr AIPS 3: finish AIPS 3: AIPS 3: procedure guesintt AIPS 3: scalar intcst,intavr,intmod,intime AIPS 3: intavr=calcintt;intcst=intavr;keyword'TELESCOP';gethead AIPS 3: if (keystrng='VLA') then;intcst=1+(2/3);end AIPS 3: if (keystrng='VLBA') then;intcst=0.131072;end AIPS 3: if (intcst=intavr) then;type'UNKNOWN TELESCOPE :'!!keystrng;en d AIPS 3: if (intavr>10) then AIPS 3: $ intime=10*floor(0.5+(intavr/10)) AIPS 3: intime=10*floor(intavr/10) AIPS 3: else;if (intavr>0) then AIPS 3: intmod=mod(intavr,intcst) AIPS 3: $ intime=intcst*((intavr-intmod)/intcst+floor(0.5+(intmod/i ntcst))) AIPS 3: intime=intcst*((intavr-intmod)/intcst+floor(intmod/intcst) ) AIPS 3: else;intime=intavr;end;end;clrtemp AIPS 3: if(numtab('NX')>0)then;type char(intime)!!' SECOND INTEGRATION S (GUESS)';end AIPS 3: return intime AIPS 3: finish AIPS 3: AIPS 3: procedure checkids AIPS 3: $LOS - account for fast switching source names - check on pos, q ual, calco AIPS 3: scalar ra1a,ra1b,ra2a,ra2b,dc1a,dc1b,dc2a,dc2b,n,m,l,idx AIPS 3: scalar q1,q2 AIPS 3: string*1 co1,co2 AIPS 3: string*16 n1,n2 AIPS 3: array alist(100),blist(100) AIPS 3: inext'SU';invers 0;keyword'NUM ROW';keyvalue 0;keystrng'';gett head AIPS 3: n=keyvalue(1);idx=1;aparm 0;bparm 0;alist 0;blist 0 AIPS 3: if (n > 1) then AIPS 3: for m=1:(n-1);clrtemp AIPS 3: pixxy m,11;tabget;ra1a keyvalue(1);ra1b keyvalue(2) AIPS 3: for l=(m+1):n;clrtemp AIPS 3: pixxy l,11;tabget;ra2a keyvalue(1);ra2b keyvalue(2) AIPS 3: if (abs(ra1a-ra2a)=0) then AIPS 3: if ( abs((ra1b-ra2b)*3600*1000) < 3 ) then $ RA within 3 mas! AIPS 3: pixxy m,12;tabget;dc1a keyvalue(1);dc1b keyvalue(2) AIPS 3: pixxy l,12;tabget;dc2a keyvalue(1);dc2b keyvalue(2) AIPS 3: if (abs(dc1a-dc2a)=0) then AIPS 3: if ( abs((dc1b-dc2b)*3600*1000) < 3 ) then $ DC wi thin 3 mas! AIPS 3: pixxy m,3;tabget;q1 keyvalue(1);pixxy l,3;tabget ;q2 keyvalue(1) AIPS 3: if (q1=q2) then $ same qualifier; same calcode? AIPS 3: pixxy m,4;tabget;co1 keystrng;pixxy l,4;tabget ;co2 keystrng AIPS 3: if (co1=co2) then AIPS 3: pixxy m,1;tabget;q1 keyvalue(1) AIPS 3: pixxy l,1;tabget;q2 keyvalue(1) AIPS 3: pixxy m,2;tabget;n1 keystrng;pixxy l,2;tabge t;n2 keystrng AIPS 3: if (idx>100) then; AIPS 3: type 'TOO MANY SOURCES TO DO DSORC - DO BY HAND!' AIPS 3: type 'NEXT =.'!!char(idx)!!' DO:'!!char(l)! !'.&.'!!char(m) AIPS 3: else AIPS 3: if (length(n1)1) then;task'DSORC';n=0 AIPS 3: outname inname;outclass inclass;outseq inseq;outdisk indis k AIPS 3: while (n100)then;type'TOO MANY SOURCES FOR DSORC';error 1;end ;clrtemp AIPS 3: end AIPS 3: finish AIPS 3: AIPS 3: procedure chkobjct AIPS 3: if (( (object='1331+305') ! (object='1328+307') ) ! (object='J 1331+3030') ) AIPS 3: then; object='3C286';end AIPS 3: if (( (object='0137+331') ! (object='0134+329') ) ! (object='J 0137+3309') ) AIPS 3: then; object='3C48';end AIPS 3: if (( (object='0521+166') ! (object='0518+165') ) ! (object='J 0521+1638') ) AIPS 3: then; object='3C138';end AIPS 3: if (( (object='0542+498') ! (object='0538+498') ) ! (object='J 0542+4951') ) AIPS 3: then; object='3C147';end AIPS 3: if (( (object='1411+522') ! (object='1409+524') ) ! (object='J 1411+5212') ) AIPS 3: then; object='3C295';end;clrtemp;return AIPS 3: finish AIPS 3: AIPS 3: procedure checkbnd AIPS 3: band='';j=1 AIPS 3: while (j<9) AIPS 3: keyword='CTYPE'!!char(j);gethead;keyword='CRVAL'!!char(j);cl rtemp AIPS 3: if (keystrng='FREQ') then;gethead;j=9;else;j=j+1;end;end AIPS 3: keyvalue(1)=keyvalue(1)/1e9; AIPS 3: if ( (keyvalue(1)>38) & (keyvalue(1)<51) ) then; band='Q ';end AIPS 3: if ( (keyvalue(1)>20.4) & (keyvalue(1)<25.5) ) then; band='K ';end AIPS 3: if ( (keyvalue(1)>13.5) & (keyvalue(1)<16.3) ) then; band='U ';end AIPS 3: if ( (keyvalue(1)> 6.8) & (keyvalue(1)< 9.6) ) then; band='X ';end AIPS 3: if ( (keyvalue(1)> 4.2) & (keyvalue(1)< 5.1) ) then; band='C ';end AIPS 3: if ( (keyvalue(1)> 1.15) & (keyvalue(1)< 1.75) ) then; band='L ';end AIPS 3: if ( (keyvalue(1)>0.298) & (keyvalue(1)<0.345) ) then; band='P ';end AIPS 3: if ( (keyvalue(1)>0.072) & (keyvalue(1)<0.076) ) then; band='4 ';end;clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure chkmodel AIPS 3: error=0;sysout='';sys2com'' AIPS 3: syscom'ls -1 $AIPSTARS/ AIPS 3: sys2com(1) inname!!'.MODEL' AIPS 3: sys2com(2) ' >& /dev/null AIPS 3: system AIPS 3: finish AIPS 3: AIPS 3: procedure loadmodl AIPS 3: scalar lsidx,l AIPS 3: array lsload(5) AIPS 3: task'TABGET';getset;inext'SU';invers 0;keyvalue=0;keystrng'' AIPS 3: keyword'NUM ROW';getthead;lsidx=keyvalue(1);l=1;clrtemp AIPS 3: for i=1:lsidx AIPS 3: pixxy=i,2,0;tabget;k=length(keystrng);j=1;clrtemp AIPS 3: while (j<21) AIPS 3: if (substr(lsampcal(j),1,k)=substr(keystrng,1,k)) then AIPS 3: lsload(l)=i;j=30;l=l+1;else;j=j+1;clrtemp AIPS 3: end;end;end;lsidx=0;checkbnd;keyword'EPOCH';keyvalue=0;keystrn g='';gethead AIPS 3: if (keyvalue(1)<1999) then;lsidx=1;end AIPS 3: for j=1:(l-1) AIPS 3: object=lsampcal(j);chkobjct;clrtemp;intype'MA';outdisk=lsdis k AIPS 3: inname=object!!'_'!!band;inclass'MODEL';inseq=1;indisk=lsdis k;chkname AIPS 3: $$ if (error>0) then;type lsampcal(lsload(j))!!' MODEL ='inname ;chkmodel AIPS 3: if (error>0) then;type lsampcal(j)!!' MODEL ='inname;chkmode l AIPS 3: if(error<1)then;go calrd;if (lsidx>0) then;eposwtch;end;en d;end $ J2000 AIPS 3: end;return AIPS 3: finish AIPS 3: AIPS 3: procedure vlanew AIPS 3: clrstat;j=numtab('BP');if (j>0) then;inext'BP';invers=-1;extde st;end AIPS 3: j=numtab('CL');if (j>1) then;inext'CL';for k=2:j;invers=k;extd est;end;end AIPS 3: j=numtab('SN');if (j>0) then;inext'SN';invers=-1;extdest;end AIPS 3: j=numtab('XX');if (j>0) then;inext'XX';invers=-1;extdest;end AIPS 3: if (inclass='LINE') then AIPS 3: j=numtab('FG');if (j>1) then;inext'FG';for k=2:j;invers=k;ex tdest;end;end AIPS 3: j=numtab('CL');if (j>1) then;inext'CL';for k=2:j;invers=k;ex tdest;end;end AIPS 3: j=numtab('BP');if (j>0) then;inext'BP';invers=-1;extdest;end AIPS 3: j=numtab('PL');if (j>0) then;inext'PL';invers=-1;extdest;end AIPS 3: end;j=numtab('PL');if (j>0) then;inext'PL';invers=-1;extdest;e nd;clrtemp AIPS 3: type'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL ,XX)' AIPS 3: finish AIPS 3: AIPS 3: procedure allzap AIPS 3: chkname;if(error<1)then;for j=1:(1-error);zap;end;end;clrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure allplot AIPS 3: tvinit;j=numtab('PL');type 'NUMBER OF PLOT FILES TO SHOW ON TV :'!!char(j) AIPS 3: if (j>0) then AIPS 3: for k=1:j;plver=k;type 'PLOT'char(k)!!'/'!!char(j);go tvpl;r ead;end AIPS 3: else;type 'NOTHING TO PLOT - DONE';end AIPS 3: finish AIPS 3: AIPS 3: procedure goplt0 AIPS 3: if (lsplot>0) then;go;end AIPS 3: finish $SN only AIPS 3: procedure goplt1 AIPS 3: if (lsplot>1) then;go;end AIPS 3: finish $SN+CL AIPS 3: procedure goplt2 AIPS 3: if (lsplot>2) then;go;end AIPS 3: finish $SN+CL+BP AIPS 3: procedure goplt3 AIPS 3: if (lsplot>3) then;go;end AIPS 3: finish $CL,BP applied AIPS 3: AIPS 3: procedure calpipe(lsdisk,lsname,lsrant) AIPS 3: vnum=33;dowait=true;getidn;vlanew;j=0;clrtemp AIPS 3: if (inclass='CH 0') then;inclass'LINE';vlanew;end;clrtemp AIPS 3: if(fsw>0)then;checkids;if(inclass='CH 0')then;inclass'LINE';ch eckids;end;end AIPS 3: if ((numtab('FG')<1)&(lsflag>=0)) then AIPS 3: if (lsflag>=1) then AIPS 3: task'QUACK';getset;flagver=1;opcode'BEG';i=min(3*tint,20) AIPS 3: reason char(i)!!' SEC AUTO-QUACK';aparm=0,i/60,-1;go AIPS 3: end;task'FLAGR';getset AIPS 3: docal 2;solint=max(3*tint-2,2.7*tint);vector=-1;docrt 0;go AIPS 3: end AIPS 3: task'SNPLT';getset;inext'CL';nplots 8;optype'AMP';vput;pixrang e=0.7,1.8 AIPS 3: goplt1;task'SETJY';getset;optype'REJY';aparm=0;freqid=1;go;opt ype'CALC' AIPS 3: if (length(lscal)<>0) then AIPS 3: optype'';zerosp=lsflux,0;lsallcal=lscal,lspntcal AIPS 3: end;sources=lsampcal;go AIPS 3: task'CALIB';getset;docalib=2;refant=lsrant;aparm=3,0,0,0,0,0,4 ,0,0;calcode'' AIPS 3: solint=lsparm(2);calsour=lspntcal;snver=numtab('SN')+1;solmo de'P' AIPS 3: soltype'L1R';baddisk=lsbadd;vput;if(star>0)then;calsour'';ca lcode'*';end;go AIPS 3: if (lsmodl>0) then $ use models for ones that exist AIPS 3: loadmodl;vget calib;calsour='';in2seq=0;in2disk=lsdisk;in2cl ass'MODEL' AIPS 3: for j=1:(l-1) AIPS 3: inext'SU';pixxy=lsload(j),2,0;tabget;calsour(1)=keystrng;c lrtemp AIPS 3: pixxy=lsload(j),4,0;tabget;calcode=substr(keystrng,1,4);cl rtemp AIPS 3: object=lsampcal(j);chkobjct;in2name=object!!'_'!!band AIPS 3: vput calib;inname=in2name;inclass=in2class;inseq=in2seq;in disk=in2disk AIPS 3: $ if no model, use point with full uvrange AIPS 3: chkname;vget calib;if (error>0)then;clr2name;end;go AIPS 3: end;clrtemp AIPS 3: else;uvrange=lsparm(3),lsparm(4);calsour=lsampcal;go;end AIPS 3: vget snplt;inext'SN';optype'PHAS';goplt0;clrtemp AIPS 3: task'CLCAL';getset;freqid=1;refant=lsrant;gainuse=numtab('CL') +1 AIPS 3: snver=numtab('SN');gainver=numtab('CL');sources'';soucode''; AIPS 3: calsour=lsphacal;calcode'';vput;if(star>0)then;calsour'';cal code'*';end;go AIPS 3: calsour=lsallcal;sources=calsour;interpol'SELF' AIPS 3: if(star>0)then;calsour'';calcode'*';soucode'*';end;go AIPS 3: vget snplt;inext'CL';optype'PHAS';goplt1;clrtemp AIPS 3: vget calib;solmode'A&P';calsour=lspntcal;calcode''; AIPS 3: solint=lsparm(13)*lsparm(2);snver=numtab('SN')+1;clr2name;vput AIPS 3: if(star>0)then;calsour'';calcode'*';end;go AIPS 3: if (lsmodl>0) then AIPS 3: loadmodl;vget calib;calsour='';in2seq=0;in2disk=lsdisk;in2cl ass'MODEL' AIPS 3: for j=1:(l-1) AIPS 3: inext'SU';pixxy=lsload(j),2,0;tabget;calsour(1)=keystrng;c lrtemp AIPS 3: pixxy=lsload(j),4,0;tabget;calcode=substr(keystrng,1,4);cl rtemp AIPS 3: object=lsampcal(j);chkobjct;in2name=object!!'_'!!band;calc ode'' AIPS 3: vput calib;inname=in2name;inclass=in2class;inseq=in2seq;in disk=in2disk AIPS 3: $ if no model, use point with full uvrange AIPS 3: chkname;vget calib;if (error>0)then;clr2name;end;go AIPS 3: end;inseq=0;indisk=lsdisk;inclass'MODEL';intype'MA' AIPS 3: for j=1:(l-1) AIPS 3: object=lsampcal(j);chkobjct;inname=object!!'_'!!band;chkna me AIPS 3: if (error<1) then;zap;end;end AIPS 3: else;uvrange=lsparm(3),lsparm(4);calsour=lsampcal;go;end AIPS 3: vget snplt;inext'SN';optype'AMP';goplt0;optype'PHAS';pixrange= -20,20;goplt0 AIPS 3: task'GETJY';getset;calsour=lsampcal;snver=numtab('SN'); AIPS 3: if (star>0) then; AIPS 3: $ for j=1:lsparm(14);sources(j)='-'!!lsampcal(j);end;k=lsparm (14)+1 AIPS 3: $ if (length(lscal)>0) then;sources(k)='-'!!lscal;k=k+1;end AIPS 3: $ for j=k:(25-k+2);sources(j)=lspntcal(j-k+2);end; AIPS 3: soucode='*' AIPS 3: else AIPS 3: sources=lspntcal;if (length(lscal)>0) then;sources(11)='-'!! lscal;end AIPS 3: end;go AIPS 3: if (lscont<1) then AIPS 3: type '****************************************************** **' AIPS 3: type '** WRITE DOWN THE FLUX DENSITIES FOR YOUR CALIBRATORS **' AIPS 3: type '** (AND DO NOT FORGET THE ERRORS EITHER!) **' AIPS 3: type '****************************************************** **';read AIPS 3: end AIPS 3: vget clcal;gainver=numtab('CL');gainuse=numtab('CL')+1;snver=n umtab('SN') AIPS 3: if(star>0)then;calsour'';calcode'*';end;go;calsour=lsallcal;so urces=calsour AIPS 3: interpol'SELF';if(star>0)then;calsour'';calcode'*';soucode'*'; end;go AIPS 3: vget snplt;inext'CL';optype'AMP';goplt1;optype'PHAS';goplt1;cl rtemp AIPS 3: if (inclass='CH 0') then AIPS 3: task'TACOP';getset AIPS 3: outdisk=indisk;outname=inname;outclass'LINE';outseq=inseq; ncount=1 AIPS 3: keystrng'';inext'FG';invers=numtab('FG');if (invers>0) the n;go;end AIPS 3: inext'CL';invers=numtab('CL');keyvalue 0;outseq=inseq;vput ;go;clrtemp AIPS 3: task'BPASS';getset;inclass'LINE';calsour=lsbndcal,lsampcal;d ocal=2 AIPS 3: solint=-1;bpassprm(5)=-1;bpassprm(9)=1;baddisk=lsbadd;go;c lrtemp AIPS 3: task'POSSM';getset;inclass'LINE';bpver 0;aparm=0,1,.4,1.2,-3 0,30,0,2,3,0 AIPS 3: nplots=6;goplt2;sources=lsbndcal;docalib 2;doband 1;aparm= 1 0;aparm(9)=3 AIPS 3: antennas=lsrant,0;goplt2;nplots=0;vput;goplt2;stokes'I';an tennas=0;goplt2 AIPS 3: sources=lsampcal;goplt3 AIPS 3: vget tacop;inclass'LINE';outclass'CH 0';invers=numtab('BP'); inext'BP';go AIPS 3: end;task'TASAV';getset;outdisk=indisk;go;dowait=false;vnum=0;c lrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure calcrms AIPS 3: scalar nbas,nvis,tbw,rms,minhrs AIPS 3: keyword'GCOUNT';gethead;nvis=keyvalue(1);nbas=numbasel;j=1 AIPS 3: minhrs=nvis*tint/(nbas*3600) $ underesimate of obs hours (over estimate rms) AIPS 3: while (j<9) $ bandwidth in a channel, continuum or spectral li ne AIPS 3: keyword='CTYPE'!!char(j);gethead;keyword='CDELT'!!char(j);cl rtemp AIPS 3: if (keystrng='FREQ') then;gethead;j=9;else;j=j+1;end;end;tbw =keyvalue(1) AIPS 3: if (lsidc <> 'CH 0') then;j=1 $ continuum, multiple IFs averag ed AIPS 3: while (j<9) AIPS 3: keyword='CTYPE'!!char(j);gethead;keyword='NAXIS'!!char(j); clrtemp AIPS 3: if(keystrng='IF')then;gethead;j=9;else;j=j+1;end;end;tbw=t bw*keyvalue(1) AIPS 3: end;checkbnd;if((band='P')!(band='4'))then;tbw=tbw/3.2;else;tb w=tbw/50;end AIPS 3: tbw=sqrt(tbw*minhrs/24e6);rms=-1 AIPS 3: if (band='Q')then;rms=3.0e-5/tbw;end;if (band='K')then;rms=2.5 e-5/tbw;end AIPS 3: if (band='U')then;rms=2.0e-5/tbw;end;if (band='X')then;rms=5.3 e-6/tbw;end AIPS 3: if (band='C')then;rms=6.4e-6/tbw;end;if (band='L')then;rms=6.6 e-6/tbw;end AIPS 3: if (band='P')then;rms=1.7e-4/tbw;end;if (band='4')then;rms=1.5 e-2/tbw;end AIPS 3: if (rms<0) then;type 'CANNOT CALCULATE RMS FROM OBSERVING BAND ..';end AIPS 3: typ 'ESTIMATED RMS:' char(rms*1000)!!' MILLI JANSKY' AIPS 3: return rms AIPS 3: finish AIPS 3: AIPS 3: procedure setboxfle AIPS 3: scalar ci,bi AIPS 3: string*48 fbox AIPS 3: fbox'/tmp/SETFC@ AIPS 3: fbox=fbox!!inname!!'_'!!inclass!!'.'!!char(inseq)!!'-'!!char(i ndisk) AIPS 3: ci=0;bi=length(fbox) AIPS 3: while(ci& /dev/null AIPS 3: if(substr(boxfile,1,1)<>' ')then;system;end;clrtemp AIPS 3: finish AIPS 3: AIPS 3: procedure catboxfile AIPS 3: sys2com'';syscom 'cat AIPS 3: sys2com(1) 'X'!!boxfile;substr(sys2com(1),1,1)='' AIPS 3: if(substr(expmsg,1,1)<>'')then;sysout=expmsg;else;sysout'';end ;clrtemp AIPS 3: system AIPS 3: finish AIPS 3: AIPS 3: procedure setimsize AIPS 3: scalar szf, kk AIPS 3: string*48 bxf AIPS 3: array szc(2), szi(2), orgc(2), orgi(2) AIPS 3: vput imagr;task'SETFC';sources'';bcount=1;bxf=setboxfle;boxfil e=bxf AIPS 3: bparm=0;infile='';shift=0;flux=0;pbparm=0.25,0;delboxfle AIPS 3: orgc=cellsize;cellsize=0;orgi=lsparm(6);imsize=0;kk=1 AIPS 3: while (kk<9) AIPS 3: keyword='CTYPE'!!char(kk);gethead;keyword='CRVAL'!!char(kk); clrtemp AIPS 3: if (keystrng='FREQ') then;gethead;kk=9;else;kk=kk+1;end;end AIPS 3: keyvalue(1)=keyvalue(1)/1e9;bparm(1)=0.375/keyvalue(1);bparm(4 )=3*bparm(1) AIPS 3: bparm(2)=30;bparm(3)=1;bparm(5)=0.031;bparm(6)=256;bparm(7)=25 6;bparm(8)=100 AIPS 3: go;szf=nfield;szc=cellsize;szi=imsize AIPS 3: vget imagr;if(lsparm(5)<0)then;cellsize=szc;else;cellsize=orgc ;end AIPS 3: if(lsparm(6)<0)then;imsize=256;nfield=szf;boxfile=bxf;else;ims ize=orgi;end AIPS 3: vput imagr AIPS 3: finish AIPS 3: AIPS 3: procedure imapipe(k,lsdisk,lsname) AIPS 3: vnum=33;dowait=true AIPS 3: if (k=1) then AIPS 3: task'SPLIT';getset;outdisk=indisk;outclass=inclass;docalib=2 AIPS 3: baddisk=lsbadd;douvcomp=-1;go AIPS 3: if (inclass='CH 0') then;inclass'LINE';outclass=inclass;doba nd=1;bpver=0 AIPS 3: go;end;end;clrtemp AIPS 3: task'TABGET';getset;inext'SU';invers=0;keyvalue=0;keystrng'';v put;clrtemp AIPS 3: task'IMAGR';getset;outdisk=indisk;flux=lsparm(8);baddisk=lsbad d;j=1 AIPS 3: while (j<9) AIPS 3: keyword='CTYPE'!!char(j);gethead;keyword='CRVAL'!!char(j);cl rtemp AIPS 3: if (keystrng='FREQ') then;gethead;j=9;else;j=j+1;end;end AIPS 3: cellsize=1.75e10/(keyvalue(1)*abs(lsparm(5)));do3dimag=1;overl ap=2;vput AIPS 3: keyword'NUM ROW';inext'SU';invers=0;keystrng'';getthead;clrtem p AIPS 3: for i=1:keyvalue(1) $ check if source is in index and uvfile e xists AIPS 3: vget tabget;pixxy=i,2,0;tabget;vget imagr;inname=keystrng;j= 1;intype'UV' AIPS 3: inseq=0;chkname;type ' ';niter=lsparm(7);lstarg=1;clrtemp;vp ut AIPS 3: if (error < 1) then $ source file exists, but same source nu mber ? AIPS 3: vget tabget;pixxy=i,1,0;tabget;error=1;k=1 AIPS 3: while ((lssid(k)>0) & (k<1001)) AIPS 3: if (lssid(k)=keyvalue(1))then error=0;end AIPS 3: k=k+1;end;end;vget imagr AIPS 3: if (error < 1) then AIPS 3: if ((lsparm(7)=1e6)&(lsparm(8)<0))then;flux=6*calcrms;end AIPS 3: if ((lsparm(6)<0)!(lsparm(5)<0))then;setimsize;else;imsize =lsparm(6);end AIPS 3: while (j<30) AIPS 3: k=length(inname) AIPS 3: if (substr(lsallcal(j),1,k)=substr(inname,1,k)) then $ c alibrator AIPS 3: lstarg=0;j=30 AIPS 3: if(lsparm(6)>=-0.99)then;niter=min(500,lsparm(7)) AIPS 3: nfield=1;boxfile'';imsize=min(256,lsparm(6)) AIPS 3: if(imsize(1)<0)then;imsize=256;end;end AIPS 3: else;j=j+1;end $ check next source, if not found -> targ et AIPS 3: end;if(substr(boxfile,1,1)<>' ')then;catboxfile;end AIPS 3: AIPS 3: j=1 AIPS 3: $calibrator lstarg=0 AIPS 3: $target if lstarg=1 AIPS 3: AIPS 3: AIPS 3: while (j<9) AIPS 3: keyword='CTYPE'!!char(j);gethead;keyword='NAXIS'!!char(j );clrtemp AIPS 3: if (keystrng='IF') then;gethead;j=9;else;j=j+1;end;end AIPS 3: type ' NOW STARTING WITH SOURCE :'!!char(i)!!' ='!! inname;type ' ' AIPS 3: if (inclass='CH 0') then AIPS 3: for k=1:keyvalue(1);bif=k;eif=k AIPS 3: if ((lstarg>0)!(lsparm(9)>0)) then;go;end AIPS 3: end;clrtemp;k=keyvalue(1) AIPS 3: inclass'LINE';keyvalue=0;keystrng'';j=1;chkname AIPS 3: if (error < 1) then AIPS 3: while (j<9) AIPS 3: keyword='CTYPE'!!char(j);gethead;clrtemp AIPS 3: if (keystrng='FREQ') then AIPS 3: keyword='NAXIS'!!char(j);gethead;echan=keyvalue(1) ;j=9 AIPS 3: else;j=j+1;end AIPS 3: end;bchan=floor(echan/10);echan=ceil(echan*9/10) AIPS 3: if (bchan=1) then;bchan=2;end;j=k AIPS 3: for k=1:j;bif=k;eif=k;if ((lstarg>0)!(lsparm(9)>1)) then;go;end AIPS 3: end;end;clrtemp AIPS 3: else AIPS 3: bif=1;eif=keyvalue(1);vput;out2disk=indisk AIPS 3: if ( (lsparm(10)=0) ! ((lsparm(9)<1)&(lstarg<1)) )then;g o;clrtemp AIPS 3: else AIPS 3: solint=lsparm(2);dotv=1;nmaps=lsparm(10);refant=lsrant ;aparm=4,0 AIPS 3: if (lsparm(10)<0) then;dotv=-1;nmaps=-1*nmaps;end;go s cimg;clrtemp AIPS 3: end;end;boxfile=setboxfle;delboxfle AIPS 3: inclass'IMAGR';inseq=0;intype'UV';indisk=lsdisk;allzap AIPS 3: $ inclass'SCIMG';allzap AIPS 3: inclass'IBM*';intype'MA';allzap AIPS 3: inclass'RBM*';allzap;inclass'LBM*';allzap;recat;clrtemp AIPS 3: else;type ' NO UV-FILE, SKIPPING SOURCE :'!!inname!!' =#' !!char(i) AIPS 3: end;end;dowait=false;vnum=0 AIPS 3: finish AIPS 3: AIPS 3: procedure avlapipe AIPS 3: tput avlapipe;vnum=33;vput avlapipe;pipeinpt;clrtemp AIPS 3: if (lserr <> 0) then; type '*** ERROR - ARE ALL INPUTS SET PRO PERLY ? ***' AIPS 3: else;lsclrcal;tint=guesintt;clrtemp AIPS 3: if (tint > 0) then;calpipe(lsdisk,lsname,lsrant);clrtemp AIPS 3: if (lsparm(1)>0) then;imapipe(1,lsdisk,lsname) AIPS 3: else;type'CALIBRATION DONE - SKIPPING SPLIT AND IMAGING' AIPS 3: type'--------------------------------------------------- --------' AIPS 3: end;type ' ' AIPS 3: if (lsplot>0) then;type 'VIEW CAL-PLOTS WITH GETSET;ALLPLO T';end;type ' ' AIPS 3: else;type '* * *';type 'SINGLE DISH VLBI EXPERIMENT?';type ' * * *';end AIPS 3: end;tget avlapipe;vnum=0;type'* APPEARS TO HAVE ENDED SUCCESSF ULLY *';clrtemp AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: default'AVLAPIPE' AIPS 3: Found in Version=ABIN AIPS 3: indisk 1; doalign -1; flagver 2; domodel 1 AIPS 3: docal 1; sources '*''' AIPS 3: $ to be set by itself later AIPS 3: solint 1; factor 5; doarray -1; imsize -1 AIPS 3: $imsize 512;$niter -1;cutoff -1;plver 0 AIPS 3: niter -1; cutoff -1 AIPS 3: $ for now debugging AIPS 3: docont 1; plver -1; doall 1; doresid 0 AIPS 3: AIPS 3: $ defaults AIPS 3: $ BADDISK 0$ INDISK 0$ DOCAT 1$ INNAME ' '$ INCLASS ' '$ INSEQ 0 AIPS 3: $ DOALIGN 1$ FLAgver 0$ SOLINT 0$ FACTOR 0$ REFANT 0$ DOMODEL -1 AIPS 3: $ KEYSTRNG ' '$ FLUX 0$ UVRANGE 0, 0$ SOURCES ' '$ CALSOUR ' ' AIPS 3: $ dopol 0$ bpa 0$ DOCONT 1$ PLVER 0$ DOALL -1$ DOARRAY -1 AIPS 3: $ IMSIZE 0, 0$ NITER 0$ CUTOFF 0$ DOCAL 0$ DORESID -1 >>::::>AIPS 3: 'AK485_2000JAN28_1' >>AIPS 3: 'AK485_2000JAN28_1' >AIPS 3: Found in Version=ABIN AIPS 3: $ Lorant Sjouwerman, versions 1.. 2005, for NRAO AIPS 3: AIPS 3: $$ General catalog looks like AIPS 3: $$ Multi-source UV data file AIPS 3: $$ Multi-source TASAV file AIPS 3: $$ Single-source calibrated data - auvf AIPS 3: $$ Single-source calibrated images- aimg AIPS 3: AIPS 3: $May need to redefine after a restore 0: AIPS 3: $allzap AIPS 3: $calcintt AIPS 3: $guesintt AIPS 3: $lsparm(5);tint;lsdisk AIPS 3: AIPS 3: procedure flatfov AIPS 3: $LOS - compile flatn-ed radius blank-ed images out to where pbco rr=2.5 (=xpb) AIPS 3: scalar uvi,mai,fov,frq,kk,tbw,tint,xpb,xcst,,fbw,fta;xpb=2.5 AIPS 3: clrname;indisk=lsdisk;intype'UV';chkname;uvi=1-error AIPS 3: if(uvi<3)then;type'ERROR: NO FILES PROCESSED !';else AIPS 3: if(uvi<4)then;type'WARNING: ONLY ONE UV-FILE - MAYBE CHECK?' ;end AIPS 3: getname 1;tint=guesintt;xcst=sqrt((3/ln(2))*(xpb-1)/xpb);kk= 1 AIPS 3: while (kk<5) AIPS 3: keyvalue=0;keystrng'';keyword='CTYPE'!!char(kk);gethead AIPS 3: if(substr(keystrng,1,4)='FREQ')then;keyword='CRVAL'!!char( kk) AIPS 3: keystrng'';gethead;frq=keyvalue(1);kk=5;else;kk=kk+1;end AIPS 3: end AIPS 3: for i=3:uvi;getname i AIPS 3: task'TABGET';inext'FQ';invers 1;keyword'NUM ROW';keystrng' ';getthead AIPS 3: for j=1:keyvalue(1) AIPS 3: pixxy=j,4,1;tabget;tbw=keyvalue(1) AIPS 3: pixxy=j,4,2;tabget;tbw=max(tbw,keyvalue(1)) AIPS 3: $ Actually imagr takes care of some of this bandwidth issue alre ady AIPS 3: $ so instead of maximum frequency span, use max individual bandw idth AIPS 3: end;inty'MA';inseq=0;inclass'*001';chkname;mai=1-error AIPS 3: if(mai>1)then;type'WARNING: MULTIPLE IMAGES - MAYBE CHECK? ';end AIPS 3: for j=1:mai $ assume inseq starts at 1.. AIPS 3: inseq=j;kk=1;cellsize=0;userid=0 AIPS 3: while (kk<5) AIPS 3: keyvalue=0;keystrng'';keyword='CTYPE'!!char(kk);gethea d AIPS 3: keyword='CDELT'!!char(kk);clrtemp AIPS 3: if(substr(keystrng,1,3)='RA-')then;gethead;cellsize(1)=k eyvalue(1);end AIPS 3: if(substr(keystrng,1,4)='DEC-')then;gethead;cellsize(2)= keyvalue(1);end AIPS 3: if(substr(keystrng,1,4)='FREQ')then;keyword='CRVAL'!!cha r(kk) AIPS 3: keystrng'';gethead;fov=keyvalue(1)/1e9;fov=1350/fov; end;kk=kk+1 AIPS 3: end;cellsize(1)=-1*cellsize(1)*3600;cellsize(2)=cellsize (2)*3600 AIPS 3: fta=min(1.75e10/(frq*abs(lsparm(5))),(min(cellsize(1),ce llsize(2)))) AIPS 3: fbw=xcst*3*fta*frq/tbw $ radius field/view due bandwidth AIPS 3: fta=xcst*3*fta/(tint*7.2722e-5) $ radius field/view due averaging AIPS 3: fov=min(fov,fbw);fov=min(fov,fta) $ min field/view ra dius, arcsec AIPS 3: imsize(1)=ceil(2*fov/cellsize(1));imsize(2)=ceil(2*fov/c ellsize(2)) AIPS 3: task'FLATN';inclass'?CL*';chkname;nfield=1-error;nmaps=1 ;clroname AIPS 3: outname=inname;coordina=0;reweight=0;doweight=0;edgskp=1 5;aparm=0 AIPS 3: pbparm=1/xpb,0;type'MINIMUM FOV :'!!char(fov)!!' ARCSEC RADIUS' AIPS 3: inclass'?CL001';go;wait;inclass'?CL*';allzap;recat;incla ss'FLATN' AIPS 3: tput;default blank;tget flatn;task'BLANK';opcode'RADI';d parm fov,0 AIPS 3: go;wait;allzap;recat AIPS 3: end;end;end AIPS 3: finish AIPS 3: AIPS 3: procedure nvasimage AIPS 3: $LOS - Determine noise, do primary beam correction, include copy right AIPS 3: scalar numfle,ll,mm AIPS 3: clrname;indisk=lsdisk;recat;chkname;numfle=1-error;mai=0 AIPS 3: while (intype<>'MA');mai=mai+1;getname mai;end AIPS 3: for j=mai:numfle;default imean;docat=1;getn j;keyvalue=0;keyst rng'' AIPS 3: keyword='CRPIX1';gethead;ll=keyvalue(1);keyword='CRPIX2';get head AIPS 3: mm=keyvalue(1);doinvers=1;blc(1)=ll-29;blc(2)=mm-30;trc(1)=l l+30 AIPS 3: trc(2)=mm+29;imstat;doinv=-1;blc=0;trc=0;rms=pixstd;go;wa AIPS 3: if(pixstd=rms)then;keyword'ACTNOISE';keytype'R';keyvalue=rms ,0;puthead;end AIPS 3: end AIPS 3: default'PBCOR';indisk=lsdisk;inclass'BLANK';chkname;pbparm=1/x pb,0 AIPS 3: for j=mai:numfle AIPS 3: getname mai;getoname mai;outclass'RADCOR';outseq=0;inclass'B LANK';chkname AIPS 3: if(error<1)then;outdisk=indisk;go;wait;zap;recat;end $ icl.. .->blanked file AIPS 3: end;default'CPYRT';indisk=lsdisk;recat;infile='AVLA:Arch_Cprt AIPS 3: for j=mai:numfle $ can only do on MA files AIPS 3: getname mai;getoname mai;outclass'NVAS06';go;wait;zap;recat AIPS 3: end AIPS 3: finish AIPS 3: AIPS 3: procedure nvasname AIPS 3: $LOS - makes the RA/Dec directory and returns the archive file n ame AIPS 3: scalar ki,ra1,ra2,dc1,dc2,st1,st2,nu1,nu2,bw,rh,rm,rs,dd,dm,ds ,rmsv,sbmv AIPS 3: string*1 pm,rmsc AIPS 3: string*2 zz AIPS 3: string*3 mmm AIPS 3: string*4 rmss,sbms,fras AIPS 3: string*5 radi AIPS 3: string*30 dir AIPS 3: string*20 expn AIPS 3: ki=1;userid=0 AIPS 3: while (ki<9) AIPS 3: keyvalue=0;keystrng'';keyword='CTYPE'!!char(ki);gethead AIPS 3: typ ki, keys AIPS 3: if(substr(keystrng,1,2)='RA')then AIPS 3: keyword='CRVAL'!!char(ki);gethead;ra1=keyvalue(1)/15;ra2=k eyvalue(2)/15 AIPS 3: keyword='CDELT'!!char(ki);gethead;cellsize(1)=-1*keyvalue( 1)*3600 AIPS 3: rh=floor(ra1);ra1=(ra1-rh)*60;rm=floor(ra1);ra1=(ra1-rm)*6 0 AIPS 3: rs=((floor((ra1+(3600*ra2))*1000)+5)/1000);clrtemp AIPS 3: $ if ((ra1+(3600*ra2))<10) then;rs=substr(char(ra1+(3600*ra 2)+0.005),1,3) AIPS 3: $ else;rs=substr(char(ra1+(3600*ra2)+0.005),1,4);end AIPS 3: if(abs(rs-floor(rs))<0.1)then;zz='.0';else;zz='';end;clrte mp AIPS 3: keyword='NAXIS'!!char(ki);gethead;ra1=0.5*keyvalue(1)*cell size(1);end AIPS 3: typ 'HERE' AIPS 3: if(substr(keystrng,1,3)='DEC')then AIPS 3: keyword='CRVAL'!!char(ki);gethead;dc1=keyvalue(1);dc2=keyv alue(2) AIPS 3: keyword='CDELT'!!char(ki);gethead;cellsize(2)=keyvalue(1)* 3600 AIPS 3: if(dc1<0)then;pm='-';dc1=-1*dc1;dc2=-1*dc2;else;pm='+';end AIPS 3: dd=floor(dc1);dc1=(dc1-dd)*60;dm=floor(dc1);dc1=(dc1-dm)*6 0 AIPS 3: ds=floor(dc1+(3600*dc2));clrtemp AIPS 3: keyword='NAXIS'!!char(ki);gethead;dc1=0.5*keyvalue(1)*cell size(2);end AIPS 3: if(substr(keystrng,1,4)='FREQ')then AIPS 3: keyword='CRVAL'!!char(ki);gethead;nu1=keyvalue(1)/1e6;nu2= keyvalue(2)/1e6 AIPS 3: keyword='CDELT'!!char(ki);gethead;bw=keyvalue(1)/1e6;end;c lrtemp AIPS 3: if(substr(keystrng,1,6)='STOKES')then AIPS 3: keyword='CRVAL'!!char(ki);gethead;st1=keyvalue(1) AIPS 3: keyword='CRPIX'!!char(ki);gethead;st2=keyvalue(1);clrtemp AIPS 3: end; AIPS 3: typ ki 'TOO' AIPS 3: if(substr(keystrng,1,1)='')then;ki=10;else;ki=ki+1;end AIPS 3: end;clrtemp $ build the output file name here AIPS 3: typ 'BUILD NOW' AIPS 3: if (intype='MA')then; $read conv size, rms from header, use im si*cell/2 for R AIPS 3: radi='S';ra2=0.5*(ra1+dc1-9);if(ra2>60)then;radi='M';ra2=ra2 /60;end $ R-fov AIPS 3: if(ra2>60)then;radi='D';ra2=ra2/60;end;radi=substr(char(ra2) ,1,4)!!radi AIPS 3: keyword='BMAJ';gethead;sbmv=keyvalue(1);keyword='BMIN';gethe ad AIPS 3: sbmv=1800*(sbmv+keyvalue(1));sbms=substr(char(sbmv),1,4) AIPS 3: AIPS 3: AIPS 3: AIPS 3: keyvalue=0;keystrng'';keyword='ACTNOISE';gethead;rmsv=keyval ue(1) $ RMS<1e4 AIPS 3: if(rmsv>1)then;rmsc='J';rmss=substr(char(rmsv),1,4);else;rms v=rmsv*1000 AIPS 3: if(rmsv>1)then;rmsc='M';rmss=substr(char(rmsv),1,4);else;r msv=rmsv*1000 AIPS 3: if(rmsv>1)then;rmsc='U';rmss=substr(char(rmsv),1,4);else AIPS 3: rmsv=rmsv*1000;rmsc='N';rmss=substr(char(rmsv),1,4) AIPS 3: end;end;end;clrtemp;fras='';sys2com(1)=' $aimg/ AIPS 3: else AIPS 3: ;clrtemp;sbms='';rmss='';rmsc='';sys2com(1)=' $auvf/ AIPS 3: end AIPS 3: AIPS 3: if (expnm='') then AIPS 3: keyword'OBSERVER';gethead;expnm=keystrng;keyword'DATE-OBS';get head AIPS 3: mmm=substr(keystrng,5,6) AIPS 3: if(mmm='01')then;mmm='JAN';end;if(mmm='02')then;mmm='FEB';end AIPS 3: if(mmm='03')then;mmm='MAR';end;if(mmm='04')then;mmm='APR';end AIPS 3: if(mmm='05')then;mmm='MAY';end;if(mmm='06')then;mmm='JUN';end AIPS 3: if(mmm='07')then;mmm='JUL';end;if(mmm='08')then;mmm='AUG';end AIPS 3: if(mmm='09')then;mmm='SEP';end;if(mmm='10')then;mmm='OCT';end AIPS 3: if(mmm='11')then;mmm='NOV';end;if(mmm='12')then;mmm='DEC';end AIPS 3: expnm=expnm!!'_'!!substr(keystrng,1,4)!!mmm!!substr(keystrng,7 ,8)!!'_X' AIPS 3: end AIPS 3: outfile=sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print outf AIPS 3: AIPS 3: $ make the source dir here AIPS 3: dir='';sysout'';syscom'mkdir AIPS 3: if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(rm );end AIPS 3: if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=cha r(rs)!!zz;end AIPS 3: $ sys2com(4)=substr(sys2com(4),1,4) AIPS 3: if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm! !char(dd);end AIPS 3: if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(dm );end AIPS 3: if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2coQUACK3: Task QUACK (release of 31DEC06) begins QUACK3: Flagged 4.33 min. of data in 26 scans QUACK3: Appears to have ended successfully QUACK3: auto 31DEC06 TST: Cpu= 0.0 Real= 0 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes FLAGR3: Task FLAGR (release of 31DEC06) begins FLAGR3: Copied FG file from vol/cno/vers 1 1 1 to 1 1 2 FLAGR3: Overall average amp= 7.613E-02 +- 8.772E-04 source= 0509+101 FLAGR3: Overall average rms= 1.572E-03 +- 1.216E-04 source= 0509+101 FLAGR3: Overall average amp= 2.547E-03 +- 2.414E-04 source= G991216 FLAGR3: Overall average rms= 1.056E-03 +- 6.556E-05 source= G991216 FLAGR3: Overall average amp= 3.394E-01 +- 3.017E-02 source= 0137+331 FLAGR3: Overall average rms= 1.740E-03 +- 1.682E-04 source= 0137+331 FLAGR3: Found 1 bad times, 140 total flags FLAGR3: Wrote 0 antenna & IF independent flags FLAGR3: Wrote 1 antenna independent, IF dependent flags FLAGR3: Wrote 139 antenna & IF dependent flags FLAGR3: Wrote 0 antenna & IF dependent, all-times flags FLAGR3: Appears to have ended successfully FLAGR3: auto 31DEC06 TST: Cpu= 5.5 Real= 22 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes SETJY3: Task SETJY (release of 31DEC06) begins SETJY3: / Resetting flux information to zero SETJY3: BIF = 1 EIF = 2 /Range of IFs SETJY3: SOURCES = '' /All sources selected SETJY3: Appears to have ended successfully SETJY3: auto 31DEC06 TST: Cpu= 0.0 Real= 0 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes SETJY3: Task SETJY (release of 31DEC06) begins SETJY3: A source model for this calibrator may be available SETJY3: Use the verb CALDIR to see if there is one SETJY3: A source model for this calibrator may be available SETJY3: Use the verb CALDIR to see if there is one SETJY3: / Flux calculated using known spectrum SETJY3: BIF = 1 EIF = 2 /Range of IFs SETJY3: '0137+331 ' IF = 1 FLUX = 3.1637 (Jy calcd) SETJY3: '0137+331 ' IF = 2 FLUX = 3.1449 (Jy calcd) SETJY3: / Using (1999.2) VLA or Reynolds (1934-638) coefficients SETJY3: Appears to have ended successfully SETJY3: auto 31DEC06 TST: Cpu= 0.0 Real= 0 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes CALIB3: Task CALIB (release of 31DEC06) begins CALIB3: CALIB USING 20000128 . X BAND . 1 DISK= 1 USID=**** CALIB3: L1 Solution type CALIB3: Selecting, editing and calibrating the data CALIB3: Doing cal transfer mode with point model for each source CALIB3: This is not self-calibration CALIB3: Dividing data by source flux densities CALIB3: Determining solutions CALIB3: Writing SN table 1 CALIB3: Found 1512 good solutions CALIB3: Average closure rms = 0.0111 +- 0.0031 CALIB3: Fraction of times having data > 2.5 rms from solution CALIB3: 0.16071 of the times had 0 - 2 percent outside 2.5 times rms CALIB3: 0.50000 of the times had 2 - 4 percent outside 2.5 times rms CALIB3: 0.07143 of the times had 4 - 6 percent outside 2.5 times rms CALIB3: 0.05357 of the times had 6 - 8 percent outside 2.5 times rms CALIB3: 0.03571 of the times had 8 - 10 percent outside 2.5 times rms CALIB3: 0.14286 of the times had 10 - 12 percent outside 2.5 times rms CALIB3: 0.03571 of the times had 12 - 14 percent outside 2.5 times rms CALIB3: Adjusting solutions to a common reference antenna CALIB3: Appears to have ended successfully CALIB3: auto 31DEC06 TST: Cpu= 0.4 Real= 1 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null CALRD3: Task CALRD (release of 31DEC06) begins CALRD3: Reading disk file AIPSTARS:3C48_X.MODEL CALRD3: Create 3C48_X .MODEL . 1 (MA) on disk 1 cno 2 CALRD3: Appears to have ended successfully CALRD3: auto 31DEC06 TST: Cpu= 0.0 Real= 0 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes CALIB3: Task CALIB (release of 31DEC06) begins CALIB3: CALIB USING 20000128 . X BAND . 1 DISK= 1 USID=**** CALIB3: L1 Solution type CALIB3: Selecting, editing and calibrating the data CALIB3: Doing self-cal mode with CC model CALIB3: SETGDS: imaging done with reprojected tangent point(s) CALIB3: FACSET: source model will be scaled to 3.164 Jy CALIB3: FACSET: 3.429181 Jy found from 300 components CALIB3: FACSET: scaling factor set to 9.22586E-01 CALIB3: VISDFT: Begin DFT component division CALIB3: VISDFT: Model components of type Point CALIB3: I Polarization model processed CALIB3: Model computation is 30 percent complete CALIB3: Model computation is 70 percent complete CALIB3: Model computation is 100 percent complete CALIB3: FACSET: source model will be scaled to 3.145 Jy CALIB3: FACSET: 3.429181 Jy found from 300 components CALIB3: FACSET: scaling factor set to 9.17087E-01 CALIB3: VISDFT: Begin DFT component division CALIB3: I Polarization model processed CALIB3: Field 1 used 300 CCs CALIB3: Determining solutions CALIB3: Deleted 54 records from SN table no. 1 CALIB3: Writing SN table 1 CALIB3: Found 216 good solutions CALIB3: Average closure rms = 0.0031 +- 0.0004 CALIB3: Fraction of times having data > 2.5 rms from solution CALIB3: 0.12500 of the times had 0 - 2 percent outside 2.5 times rms CALIB3: 0.50000 of the times had 2 - 4 percent outside 2.5 times rms CALIB3: 0.37500 of the times had 4 - 6 percent outside 2.5 times rms CALIB3: Adjusting solutions to a common reference antenna CALIB3: Appears to have ended successfully CALIB3: auto 31DEC06 TST: Cpu= 1.1 Real= 4 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes CLCAL3: Task CLCAL (release of 31DEC06) begins CLCAL3: Using interpolation mode 2PT CLCAL3: Processing SN table 1 CLCAL3: SNMRG: Merging SN table CLCAL3: SNMRG: Write 378 merged records from 378 input records CLCAL3: SN2CL: Applying SN tables to CL table 1, writing CL table 2 CLCAL3: Appears to have ended successfully CLCAL3: auto 31DEC06 TST: Cpu= 0.4 Real= 1 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes CLCAL3: Task CLCAL (release of 31DEC06) begins CLCAL3: Using interpolation mode SELF CLCAL3: Deleted 702 records from CL table no. 2 CLCAL3: Processing SN table 1 CLCAL3: WARNING: SN table 1 has already been applied CLCAL3: SNMRG: Merging SN table CLCAL3: SNMRG: Write 378 merged records from 378 input records CLCAL3: SN2CL: Applying SN tables to CL table 1, writing CL table 2 CLCAL3: Appears to have ended successfully CLCAL3: auto 31DEC06 TST: Cpu= 0.2 Real= 1 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes CALIB3: Task CALIB (release of 31DEC06) begins CALIB3: CALIB USING 20000128 . X BAND . 1 DISK= 1 USID=**** CALIB3: L1 Solution type CALIB3: Selecting, editing and calibrating the data CALIB3: Doing cal transfer mode with point model for each source CALIB3: This is not self-calibration CALIB3: Dividing data by source flux densities CALIB3: Determining solutions CALIB3: Writing SN table 2 CALIB3: RPOL, IF= 1 The average gain over these antennas is 3.660E+00 CALIB3: RPOL, IF= 2 The average gain over these antennas is 3.662E+00 CALIB3: LPOL, IF= 1 The average gain over these antennas is 3.665E+00 CALIB3: LPOL, IF= 2 The average gain over these antennas is 3.668E+00 CALIB3: Found 1404 good solutions CALIB3: Average closure rms = 0.0014 +- 0.0003 CALIB3: Fraction of times having data > 2.5 rms from solution CALIB3: 0.57407 of the times had 0 - 2 percent outside 2.5 times rms CALIB3: 0.03704 of the times had 2 - 4 percent outside 2.5 times rms CALIB3: 0.01852 of the times had 4 - 6 percent outside 2.5 times rms CALIB3: 0.12963 of the times had 6 - 8 percent outside 2.5 times rms CALIB3: 0.07407 of the times had 8 - 10 percent outside 2.5 times rms CALIB3: 0.05556 of the times had 10 - 12 percent outside 2.5 times rms CALIB3: 0.03704 of the times had 12 - 14 percent outside 2.5 times rms CALIB3: Adjusting solutions to a common reference antenna CALIB3: Appears to have ended successfully CALIB3: auto 31DEC06 TST: Cpu= 1.2 Real= 6 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes CALIB3: Task CALIB (release of 31DEC06) begins CALIB3: CALIB USING 20000128 . X BAND . 1 DISK= 1 USID=**** CALIB3: L1 Solution type CALIB3: Selecting, editing and calibrating the data CALIB3: Doing self-cal mode with CC model CALIB3: SETGDS: imaging done with reprojected tangent point(s) CALIB3: FACSET: source model will be scaled to 3.164 Jy CALIB3: FACSET: 3.429181 Jy found from 300 components CALIB3: FACSET: scaling factor set to 9.22586E-01 CALIB3: VISDFT: Begin DFT component division CALIB3: VISDFT: Model components of type Point CALIB3: I Polarization model processed CALIB3: Model computation is 30 percent complete CALIB3: Model computation is 70 percent complete CALIB3: Model computation is 100 percent complete CALIB3: FACSET: source model will be scaled to 3.145 Jy CALIB3: FACSET: 3.429181 Jy found from 300 components CALIB3: FACSET: scaling factor set to 9.17087E-01 CALIB3: VISDFT: Begin DFT component division CALIB3: I Polarization model processed CALIB3: Field 1 used 300 CCs CALIB3: Determining solutions CALIB3: Deleted 27 records from SN table no. 2 CALIB3: Writing SN table 2 CALIB3: RPOL, IF= 1 The average gain over these antennas is 2.971E+00 CALIB3: RPOL, IF= 2 The average gain over these antennas is 2.974E+00 CALIB3: LPOL, IF= 1 The average gain over these antennas is 2.964E+00 CALIB3: LPOL, IF= 2 The average gain over these antennas is 2.964E+00 CALIB3: Found 108 good solutions CALIB3: Average closure rms = 0.0006 +- 0.0001 CALIB3: Fraction of times having data > 2.5 rms from solution CALIB3: 0.25000 of the times had 0 - 2 percent outside 2.5 times rms CALIB3: 0.50000 of the times had 4 - 6 percent outside 2.5 times rms CALIB3: 0.25000 of the times had 6 - 8 percent outside 2.5 times rms CALIB3: Adjusting solutions to a common reference antenna CALIB3: Appears to have ended successfully CALIB3: auto 31DEC06 TST: Cpu= 1.1 Real= 4 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 GETJY3: Task GETJY (release of 31DEC06) begins GETJY3: Source:Qual CALCODE IF Flux (Jy) GETJY3: 0509+101 : 0 A 1 0.64299 +/- 0.00097 GETJY3: 2 0.64268 +/- 0.00115 GETJY3: Appears to have ended successfully GETJY3: auto 31DEC06 TST: Cpu= 0.0 Real= 0 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 AIPS 3: Resumes CLCAL3: Task CLCAL (release of 31DEC06) begins CLCAL3: Using interpolation mode 2PT CLCAL3: Processing SN table 2 CLCAL3: SNMRG: Merging SN table CLCAL3: SNMRG: Write 351 merged records from 351 input records CLCAL3: SN2CL: Applying SN tables to CL table 2, writing CL table 3 CLCAL3: Appears to have ended successfully CLCAL3: auto 31DEC06 TST: Cpu= 0.4 Real= 1 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 AIPS 3: Resumes AIPS 3: Resumes CLCAL3: Task CLCAL (release of 31DEC06) begins CLCAL3: Using interpolation mode SELF CLCAL3: Deleted 702 records from CL table no. 3 CLCAL3: Processing SN table 2 CLCAL3: WARNING: SN table 2 has already been applied CLCAL3: SNMRG: Merging SN table CLCAL3: SNMRG: Write 351 merged records from 351 input records CLCAL3: SN2CL: Applying SN tables to CL table 2, writing CL table 3 CLCAL3: Appears to have ended successfully CLCAL3: auto 31DEC06 TST: Cpu= 0.2 Real= 1 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes TASAV3: Task TASAV (release of 31DEC06) begins TASAV3: Create 20000128 .TASAV . 1 (UV) on disk 1 cno 2 TASAV3: Copied AN file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied NX file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied SU file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied FQ file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied CL file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied CL file from vol/cno/vers 1 1 2 to 1 2 2 TASAV3: Copied CL file from vol/cno/vers 1 1 3 to 1 2 3 TASAV3: Copied TY file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied WX file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied OF file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied FG file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied FG file from vol/cno/vers 1 1 2 to 1 2 2 TASAV3: Copied XX file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied SN file from vol/cno/vers 1 1 1 to 1 2 1 TASAV3: Copied SN file from vol/cno/vers 1 1 2 to 1 2 2 TASAV3: Appears to have ended successfully TASAV3: auto 31DEC06 TST: Cpu= 0.2 Real= 1 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes SPLIT3: Task SPLIT (release of 31DEC06) begins SPLIT3: You are using a non-standard program SPLIT3: Doing subarray 1 SPLIT3: Create G991216 .X BAND. 1 (UV) on disk 1 cno 3 SPLIT3: Applying CL Table version 3 SPLIT3: Previously flagged flagged by gain kept SPLIT3: Partially 7167 0 7167 SPLIT3: Fully 0 0 142840 SPLIT3: Copied AN file from vol/cno/vers 1 1 1 to 1 3 1 SPLIT3: Copied WX file from vol/cno/vers 1 1 1 to 1 3 1 SPLIT3: Copied OF file from vol/cno/vers 1 1 1 to 1 3 1 SPLIT3: Copied XX file from vol/cno/vers 1 1 1 to 1 3 1 SPLIT3: Create 0509+101 .X BAND. 1 (UV) on disk 1 cno 4 SPLIT3: Previously flagged flagged by gain kept SPLIT3: Partially 570 0 570 SPLIT3: Fully 0 0 22921 SPLIT3: Copied AN file from vol/cno/vers 1 1 1 to 1 4 1 SPLIT3: Copied WX file from vol/cno/vers 1 1 1 to 1 4 1 SPLIT3: Copied OF file from vol/cno/vers 1 1 1 to 1 4 1 SPLIT3: Copied XX file from vol/cno/vers 1 1 1 to 1 4 1 SPLIT3: Create 0137+331 .X BAND. 1 (UV) on disk 1 cno 5 SPLIT3: Previously flagged flagged by gain kept SPLIT3: Partially 52 0 52 SPLIT3: Fully 0 0 7995 SPLIT3: Copied AN file from vol/cno/vers 1 1 1 to 1 5 1 SPLIT3: Copied WX file from vol/cno/vers 1 1 1 to 1 5 1 SPLIT3: Copied OF file from vol/cno/vers 1 1 1 to 1 5 1 SPLIT3: Copied XX file from vol/cno/vers 1 1 1 to 1 5 1 SPLIT3: Appears to have ended successfully SPLIT3: auto 31DEC06 TST: Cpu= 0.6 Real= 2 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.02919 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@G991216_X,BAND.0-1 >& /dev/null SETFC3: Task SETFC (release of 31DEC06) begins SETFC3: Found G991216 X BAND Seq 1 Disk: 1 in slot 3 SETFC3: SETCEL: recommends IMSIZE 1458 CELLSIZE 0.21958 SETFC3: SETCEL: returns IMSIZE 2048 CELLSIZE 0.21958 SETFC3: ZTXOP2: using translated file name = SETFC3: ZTXOP2: /tmp/SETFC@G991216_X,BAND.0-1 SETFC3: FLYEYE added 1 fields to BOXFILE to 0.000 deg SETFC3: WARNING: THIS MAY NOT COVER THE DESIRED AREA SETFC3: Searching catalog between 0.00 and 0.13 degrees radius SETFC3: ZTXOP2: using translated file name = SETFC3: ZTXOP2: /home/auto/aips/TEXT/STARS/NV00.0030 SETFC3: No NVSS sources selected for BOXFILE SETFC3: The Sun is 128.9 deg away - ignoring SETFC3: First field number written was 1 SETFC3: Highest field number written was 1 SETFC3: returns adverbs to AIPS SETFC3: Appears to have ended successfully SETFC3: auto 31DEC06 TST: Cpu= 0.5 Real= 2 C 1 2036 2036 05 09 31.29 11 17 07.4 00001 -1 1019 1024 1025 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.02919 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@G991216_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@G991216_X,BAND.0-1 >> /home/auto/run/AK485_2000JA AIPS 3: N28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :1 =G991216' AIPS 3: ' ' IMAGR3: Task IMAGR (release of 31DEC06) begins IMAGR3: ZTXOP2: using translated file name = IMAGR3: ZTXOP2: /tmp/SETFC@G991216_X,BAND.0-1 IMAGR3: FIELDF: Final field parameters and # read are: IMAGR3: Field 1 2036 2036 5.0170E-11 6.3949E-12 0 IMAGR3: ZTXOP2: using translated file name = IMAGR3: ZTXOP2: /tmp/SETFC@G991216_X,BAND.0-1 IMAGR3: WINDF: Number of clean boxes/field read as follows: IMAGR3: Field 01: 1 IMAGR3: Create G991216 .IMAGR . 1 (UV) on disk 1 cno 6 IMAGR3: Beginning channel 1 through 1 with 2 IFs IMAGR3: IMACPY: Copied 150007 visibilities to be imaged IMAGR3: **** WARNING data included out of inner portion of UV plane **** IMAGR3: **** Watch for high-frequency & other poor cleaning effects **** IMAGR3: UVWAIT: begin finding uniform weights IMAGR3: UVWAIT: Average grid weight 1.190E+05 IMAGR3: UVWAIT: Adding temperance S 2.380E+04 IMAGR3: UVWAIT: begin applying uniform or other weights IMAGR3: UVWAIT: Sum of weights in 7.097E+08 and out 1.277E+09 IMAGR3: UVWAIT: Noise is increased by a factor 1.152 due to weighting IMAGR3: UVWAIT: Average summed weight 1.190E+05 over 299936 vis IMAGR3: Create G991216 .IBM001. 1 (MA) on disk 1 cno 7 IMAGR3: Create G991216 .ICL001. 1 (MA) on disk 1 cno 8 IMAGR3: GRDFLT: X and Y convolution type = SPHEROIDAL IMAGR3: GRDFLT: X and Y parms = 3.0000 1.0000 IMAGR3: GRDFLT: convolution function sampled every 1/100 of a cell IMAGR3: GRDMEM: Ave 2 Channels; 8.435100E+09 to 8.485100E+09 Hz IMAGR3: Field 1 Sum of gridding weights = 1.35567E+10 IMAGR3: Field 1 Beam min = -140.0 MilliJy, max = 1.0 Jy IMAGR3: Field 1 fit FWHM = 728.530 x 677.607 Milliarcsec, PA= -16.5 IMAGR3: CLBHIS: minimum component 0.431 of current peak IMAGR3: Field 1 min = -137.6 MicroJy,max = 169.3 MicroJy IMAGR3: Peak residual in window 151.387 less than limit 175.117 MicroJy IMAGR3: Field 1 min = -137.6 MicroJy,max = 169.3 MicroJy IMAGR3: Restoring Clean components IMAGR3: Checking image max/min IMAGR3: Field 1 final Clean flux 0.000 Jy IMAGR3: Deleting UV work file: IMAGR3: Destroyed 1 extension files of type AN IMAGR3: Destroyed 1 extension files of type FQ IMAGR3: Destroyed UV image file: catno= 6 disk= 1 IMAGR3: Appears to have ended successfully IMAGR3: auto 31DEC06 TST: Cpu= 5.0 Real= 20 m(7)=char(ds );end AIPS 3: sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp;for i=1:7;dir=dir!!sys2com(i);end;ki=length(dir ) $ must be 27 AIPS 3: dir=substr(dir,2,ki);if(ki<>27)then;type'WARNING: WRONG DIRECT ORY NAME ?';end AIPS 3: AIPS 3: sysout=dir!!'/'!!sbms!!','!!expnm!!','!!rmss!!rmsc!!fras!!radi AIPS 3: print sysout AIPS 3: $keep sysout - not if we use dir instead AIPS 3: syscom'';sys2com'';clrtemp AIPS 3: return AIPS 3: finish AIPS 3: AIPS 3: procedure nvasarch AIPS 3: scalar nn AIPS 3: $LOS - archives the files to disk - define $EXP (and $AVLA/$ADAT /$AIMG/$AUVF) AIPS 3: default fitab;indisk=lsdisk;recat AIPS 3: $ figure out array for uv name AIPS 3: $ getname 1; AIPS 3: for nn=mai:numfle $ archive MA files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: typ length(outfile),length(sysout) AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X$FITS/'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: $ sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sys2com(2)'X'!!dir;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: outfile='FITS:'!!outfile AIPS 3: ;go;wait; $zap AIPS 3: ;system AIPS 3: end AIPS 3: clrname;indisk=lsdisk;chkname;numfle=1-error AIPS 3: numfle=mai -1 AIPS 3: for nn=3:numfle $ archive calibrated UV files AIPS 3: getname nn AIPS 3: nvasname AIPS 3: outfile='/tmp/tempuvfits AIPS 3: go;wait; $zap AIPS 3: syscom'mv -f AIPS 3: sys2com(1)'X'!!outfile;substr(sys2com(1),1,1)='' AIPS 3: sys2com(2)'X'!!sysout;substr(sys2com(2),1,1)='' AIPS 3: sysout'';sys2com(3) ' >& /dev/null AIPS 3: system AIPS 3: end AIPS 3: getname 2 $ archive calibration tables AIPS 3: $ do not use nvasname as the dir is ADAT and dirname is expid AIPS 3: AIPS 3: sys2com'';sysout'';syscom 'mkdir AIPS 3: sys2com(1)=' $adat/ AIPS 3: AIPS 3: $ if(rh<10)then;sys2com(2)='J0'!!char(rh);else;sys2com(2)='J'!! char(rh);end AIPS 3: $ if(rm<10)then;sys2com(3)='0'!!char(rm);else;sys2com(3)=char(r m);end AIPS 3: $ if(rs<10)then;sys2com(4)='0'!!char(rs)!!zz;else;sys2com(4)=ch ar(rs)!!zz;end AIPS 3: $ if(dd<10)then;sys2com(5)=pm!!'0'!!char(dd);else;sys2com(5)=pm !!char(dd);end AIPS 3: $ if(dm<10)then;sys2com(6)='0'!!char(dm);else;sys2com(6)=char(d m);end AIPS 3: $ if(ds<10)then;sys2com(7)='0'!!char(ds);else;sys2com(7)=char(d s);end AIPS 3: AIPS 3: sys2com(1)=sys2com(1)!!expnm;sys2com(8) ' >& /dev/null AIPS 3: system;clrtemp AIPS 3: AIPS 3: finish AIPS 3: AIPS 3: procedure nvas AIPS 3: typ expid;flatfov;nvasimage AIPS 3: $nvasarch AIPS 3: finish >AIPS 3: Found in Version=ABIN AIPS 3: Found in Version=ABIN AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'AIPS WILL CHOOSE THE REFERENCE ANTENNA' AIPS 3: Got(1) disk= 1 user=**** type=UV 20000128.X BAND.1 AIPS 3: 'SETFC WILL DETERMINE THE CELL SIZE' AIPS 3: '3.3333 SECOND INTEGRATIONS (GUESS)' AIPS 3: 'DONE CLEANUP OF OLD TABLE EXTENTION FILES (CL,SN,FG,BP,PL,XX)' AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: '0137+331 MODEL =' '3C48_X' AIPS 3: SYSTEM command to be executed is: AIPS 3: ls -1 $AIPSTARS/3C48_X.MODEL >& /dev/null AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Destroyed 1 extension files of type CC AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 2 disk= 1 AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: Resumes AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.02919 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@G991216_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@G991216_X,BAND.0-1 >> /home/auto/run/AK485_2000JA AIPS 3: N28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :1 =G991216' AIPS 3: ' ' AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@G991216_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 7 disk= 1 AIPS 3: Disk 1 in-CNO 8 renumbered as CNO 6 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.07375 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null SETFC3: Task SETFC (release of 31DEC06) begins SETFC3: Found 0509+101 X BAND Seq 1 Disk: 1 in slot 4 SETFC3: SETCEL: recommends IMSIZE 1458 CELLSIZE 0.21958 SETFC3: SETCEL: returns IMSIZE 2048 CELLSIZE 0.21958 SETFC3: ZTXOP2: using translated file name = SETFC3: ZTXOP2: /tmp/SETFC@0509+101_X,BAND.0-1 SETFC3: FLYEYE added 1 fields to BOXFILE to 0.000 deg SETFC3: WARNING: THIS MAY NOT COVER THE DESIRED AREA SETFC3: Searching catalog between 0.00 and 0.13 degrees radius SETFC3: ZTXOP2: using translated file name = SETFC3: ZTXOP2: /home/auto/aips/TEXT/STARS/NV00.0030 SETFC3: Field RA Dec Flux Beam Sep SETFC3: 2 05:09:27.45 10:11:44.7 0.465 1.000 0.000 SETFC3: Add NVSS: wrote 1 fields to BOXFILE SETFC3: The Sun is 128.6 deg away - ignoring SETFC3: First field number written was 1 SETFC3: Highest field number written was 2 SETFC3: returns adverbs to AIPS SETFC3: Appears to have ended successfully SETFC3: auto 31DEC06 TST: Cpu= 0.4 Real= 1 C 1 2036 2036 05 09 27.46 10 11 44.6 00001 -1 1019 1024 1025 C 2 246 246 05 09 27.45 10 11 44.7 00002 -1 100 128 129 TFC@G991216_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 7 disk= 1 AIPS 3: Disk 1 in-CNO 8 renumbered as CNO 6 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.07375 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@0509+101_X,BAND.0-1 >> /home/auto/run/AK485_2000J AIPS 3: AN28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :2 =0509+101' AIPS 3: ' ' IMAGR3: Task IMAGR (release of 31DEC06) begins IMAGR3: ZTXOP2: using translated file name = IMAGR3: ZTXOP2: /tmp/SETFC@0509+101_X,BAND.0-1 IMAGR3: FIELDF: Final field parameters and # read are: IMAGR3: Field 1 2036 2036 4.2813E-02 6.3949E-12 0 IMAGR3: Field 2 246 246 -1.0482E-01 1.0000E-01 0 IMAGR3: ZTXOP2: using translated file name = IMAGR3: ZTXOP2: /tmp/SETFC@0509+101_X,BAND.0-1 IMAGR3: WINDF: Number of clean boxes/field read as follows: IMAGR3: Field 01: 1 Field 02: 1 IMAGR3: Create 0509+101 .IMAGR . 1 (UV) on disk 1 cno 7 IMAGR3: Beginning channel 1 through 1 with 2 IFs IMAGR3: IMACPY: Copied 23491 visibilities to be imaged IMAGR3: **** WARNING data included out of inner portion of UV plane **** IMAGR3: **** Watch for high-frequency & other poor cleaning effects **** IMAGR3: UVWAIT: begin finding uniform weights IMAGR3: UVWAIT: Average grid weight 2.380E+04 IMAGR3: UVWAIT: Adding temperance S 4.760E+03 IMAGR3: UVWAIT: begin applying uniform or other weights IMAGR3: UVWAIT: Sum of weights in 1.109E+08 and out 1.610E+08 IMAGR3: UVWAIT: Noise is increased by a factor 1.114 due to weighting IMAGR3: UVWAIT: Average summed weight 2.380E+04 over 46878 vis IMAGR3: Create 0509+101 .IBM001. 1 (MA) on disk 1 cno 8 IMAGR3: Create 0509+101 .IBM002. 1 (MA) on disk 1 cno 9 IMAGR3: Create 0509+101 .ICL001. 1 (MA) on disk 1 cno 10 IMAGR3: Create 0509+101 .ICL002. 1 (MA) on disk 1 cno 11 IMAGR3: GRDFLT: X and Y convolution type = SPHEROIDAL IMAGR3: GRDFLT: X and Y parms = 3.0000 1.0000 IMAGR3: GRDFLT: convolution function sampled every 1/100 of a cell IMAGR3: GRDMEM: Ave 2 Channels; 8.435100E+09 to 8.485100E+09 Hz IMAGR3: Field 1 Sum of gridding weights = 1.70953E+09 IMAGR3: Field 1 Beam min = -109.3 MilliJy, max = 1.0 Jy IMAGR3: Field 1 fit FWHM = 791.996 x 712.392 Milliarcsec, PA= -2.1 IMAGR3: Field 2 Sum of gridding weights = 1.70955E+09 IMAGR3: Field 2 Beam min = -109.3 MilliJy, max = 1.0 Jy IMAGR3: Field 2 fit FWHM = 791.995 x 712.392 Milliarcsec, PA= -2.1 IMAGR3: CLBHIS: minimum component 0.451 of current peak IMAGR3: Field 1 min = -70.3 MilliJy,max = 632.3 MilliJy IMAGR3: Field 2 min = -71.8 MilliJy,max = 577.3 MilliJy IMAGR3: BGC Clean: using 2043 cell beam + residuals > 28.08 MilliJy IMAGR3: 7216 Residual map points loaded IMAGR3: Field 1 min allowed flux = 272.173 MilliJy iter= 9 IMAGR3: Field 1 Clean flux density= 387.318 MilliJy 9 comps IMAGR3: Total Cleaned flux density = 387.318 MilliJy 9 comps IMAGR3: SETDO3: imaging done with multiple tangent planes IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: VISDFT: Model components of type Point IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -28.3 MilliJy,max = 247.4 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 2.353E-01 < Second best 2.587E-01 IMAGR3: Field 1 min = -28.8 MilliJy,max = 245.0 MilliJy IMAGR3: BGC Clean: using 2043 cell beam + residuals > 12.09 MilliJy IMAGR3: 5853 Residual map points loaded IMAGR3: Field 1 min allowed flux = 105.519 MilliJy iter= 19 IMAGR3: Field 1 Clean flux density= 554.032 MilliJy 19 comps IMAGR3: Total Cleaned flux density = 554.032 MilliJy 19 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -10.9 MilliJy,max = 99.0 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 9.419E-02 < Second best 1.003E-01 IMAGR3: Field 1 min = -10.9 MilliJy,max = 96.8 MilliJy IMAGR3: BGC Clean: using 2043 cell beam + residuals > 4.69 MilliJy IMAGR3: 6033 Residual map points loaded IMAGR3: Field 1 min allowed flux = 41.500 MilliJy iter= 29 IMAGR3: Field 1 Clean flux density= 619.779 MilliJy 29 comps IMAGR3: Total Cleaned flux density = 619.779 MilliJy 29 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -11.1 MilliJy,max = 40.9 MilliJy IMAGR3: BGC Clean: using 509 cell beam + residuals > 4.40 MilliJy IMAGR3: 516 Residual map points loaded IMAGR3: Field 2 min allowed flux = 17.133 MilliJy iter= 10 IMAGR3: Field 2 Clean flux density= 27.496 MilliJy 10 comps IMAGR3: Total Cleaned flux density = 647.275 MilliJy 39 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -13.8 MilliJy,max = 14.1 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.346E-02 < Second best 1.630E-02 IMAGR3: Field 2 min = -12.2 MilliJy,max = 15.7 MilliJy IMAGR3: BGC Clean: using 509 cell beam + residuals > 1.37 MilliJy IMAGR3: 3564 Residual map points loaded IMAGR3: Field 2 min allowed flux = -6.944 MilliJy iter= 43 IMAGR3: Field 2 Clean flux density= 24.379 MilliJy 43 comps IMAGR3: Total Cleaned flux density = 644.159 MilliJy 72 comps IMAGR3: ALGSTB: All 183 Rows In AP (Max 267) IMAGR3: ALGSTB field 2 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 172- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -7.9 MilliJy,max = 6.5 MilliJy IMAGR3: BGC Clean: using 527 cell beam + residuals > 1.20 MilliJy IMAGR3: 12894 Residual map points loaded IMAGR3: Field 1 min allowed flux = -3.569 MilliJy iter= 74 IMAGR3: Field 1 Clean flux density= 615.933 MilliJy 74 comps IMAGR3: Total Cleaned flux density = 640.312 MilliJy 117 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -4.2 MilliJy,max = 4.5 MilliJy IMAGR3: BGC Clean: using 151 cell beam + residuals > 1.32 MilliJy IMAGR3: 1120 Residual map points loaded IMAGR3: Field 2 min algorithm flux= -2.263 MilliJy iter= 141 IMAGR3: Field 2 Clean flux density= 27.365 MilliJy 141 comps IMAGR3: Total Cleaned flux density = 643.298 MilliJy 215 comps IMAGR3: ALGSTB: All 183 Rows In AP (Max 267) IMAGR3: ALGSTB field 2 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 172- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.9 MilliJy,max = 2.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.01 MilliJy IMAGR3: 17739 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -1.703 MilliJy iter= 276 IMAGR3: Field 1 Clean flux density= 617.231 MilliJy 276 comps IMAGR3: Total Cleaned flux density = 644.596 MilliJy 417 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -1.9 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 991.60 MicroJy IMAGR3: 615 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 1.237 MilliJy iter= 250 IMAGR3: Field 2 Clean flux density= 30.361 MilliJy 250 comps IMAGR3: Total Cleaned flux density = 647.592 MilliJy 526 comps IMAGR3: ALGSTB: All 183 Rows In AP (Max 267) IMAGR3: ALGSTB field 2 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 172- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.8 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 937.34 MicroJy IMAGR3: 19186 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 1.440 MilliJy iter= 633 IMAGR3: Field 1 Clean flux density= 604.708 MilliJy 633 comps IMAGR3: Total Cleaned flux density = 635.069 MilliJy 883 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -2.7 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 915.59 MicroJy IMAGR3: 19104 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 1.315 MilliJy iter= 1102 IMAGR3: Field 1 Clean flux density= 597.984 MilliJy 1102 comps IMAGR3: Total Cleaned flux density = 628.345 MilliJy 1352 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -2.7 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 890.42 MicroJy IMAGR3: 18981 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -1.221 MilliJy iter= 1690 IMAGR3: Field 1 Clean flux density= 589.706 MilliJy 1690 comps IMAGR3: Total Cleaned flux density = 620.067 MilliJy 1940 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -1.2 MilliJy,max = 1.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 885.46 MicroJy IMAGR3: 240 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 925.004 MicroJy iter= 334 IMAGR3: Field 2 Clean flux density= 31.328 MilliJy 334 comps IMAGR3: Total Cleaned flux density = 621.034 MilliJy 2024 comps IMAGR3: ALGSTB: All 183 Rows In AP (Max 267) IMAGR3: ALGSTB field 2 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 172- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.6 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 854.95 MicroJy IMAGR3: 19690 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -1.139 MilliJy iter= 2460 IMAGR3: Field 1 Clean flux density= 589.706 MilliJy 2460 comps IMAGR3: Total Cleaned flux density = 621.034 MilliJy 2794 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -2.5 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 828.15 MicroJy IMAGR3: 19598 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 1.068 MilliJy iter= 3382 IMAGR3: Field 1 Clean flux density= 581.554 MilliJy 3382 comps IMAGR3: Total Cleaned flux density = 612.883 MilliJy 3716 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.4 MilliJy,max = 2.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 801.24 MicroJy IMAGR3: 19509 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 1.008 MilliJy iter= 4454 IMAGR3: Field 1 Clean flux density= 577.535 MilliJy 4454 comps IMAGR3: Total Cleaned flux density = 608.863 MilliJy 4788 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.4 MilliJy,max = 2.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 773.41 MicroJy IMAGR3: 19391 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 952.733 MicroJy iter= 5679 IMAGR3: Field 1 Clean flux density= 572.518 MilliJy 5679 comps IMAGR3: Total Cleaned flux density = 603.846 MilliJy 6013 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.2 MilliJy,max = 2.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 746.90 MicroJy IMAGR3: 19259 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -904.031 MicroJy iter= 7055 IMAGR3: Field 1 Clean flux density= 573.522 MilliJy 7055 comps IMAGR3: Total Cleaned flux density = 604.850 MilliJy 7389 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 2 min = -1.1 MilliJy,max = 975.1 MicroJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 743.40 MicroJy IMAGR3: 44 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 744.813 MicroJy iter= 368 IMAGR3: Field 2 Clean flux density= 31.661 MilliJy 368 comps IMAGR3: Total Cleaned flux density = 605.183 MilliJy 7423 comps IMAGR3: ALGSTB: All 183 Rows In AP (Max 267) IMAGR3: ALGSTB field 2 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 172- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.2 MilliJy,max = 2.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 716.66 MicroJy IMAGR3: 19914 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 858.057 MicroJy iter= 8635 IMAGR3: Field 1 Clean flux density= 565.101 MilliJy 8635 comps IMAGR3: Total Cleaned flux density = 596.763 MilliJy 9003 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.1 MilliJy,max = 2.3 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 689.96 MicroJy IMAGR3: 19876 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 818.714 MicroJy iter= 10433 IMAGR3: Field 1 Clean flux density= 561.942 MilliJy 10433 comps IMAGR3: Total Cleaned flux density = 593.604 MilliJy 10801 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.0 MilliJy,max = 2.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 665.64 MicroJy IMAGR3: 19802 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 787.882 MicroJy iter= 12465 IMAGR3: Field 1 Clean flux density= 552.475 MilliJy 12465 comps IMAGR3: Total Cleaned flux density = 584.137 MilliJy 12833 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.1 MilliJy,max = 2.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 642.39 MicroJy IMAGR3: 19743 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -762.817 MicroJy iter= 14789 IMAGR3: Field 1 Clean flux density= 548.753 MilliJy 14789 comps IMAGR3: Total Cleaned flux density = 580.414 MilliJy 15157 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.0 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 622.15 MicroJy IMAGR3: 19681 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 732.450 MicroJy iter= 17442 IMAGR3: Field 1 Clean flux density= 544.119 MilliJy 17442 comps IMAGR3: Total Cleaned flux density = 575.780 MilliJy 17810 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 2 min = -1.0 MilliJy,max = 1.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 621.18 MicroJy IMAGR3: 52 Residual map points loaded IMAGR3: Field 2 min algorithm flux= -630.900 MicroJy iter= 406 IMAGR3: Field 2 Clean flux density= 31.707 MilliJy 406 comps IMAGR3: Total Cleaned flux density = 575.826 MilliJy 17848 comps IMAGR3: ALGSTB: All 183 Rows In AP (Max 267) IMAGR3: ALGSTB field 2 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 172- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -2.0 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 593.95 MicroJy IMAGR3: 19911 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -690.805 MicroJy iter= 20374 IMAGR3: Field 1 Clean flux density= 538.094 MilliJy 20374 comps IMAGR3: Total Cleaned flux density = 569.801 MilliJy 20780 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.9 MilliJy,max = 1.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 573.69 MicroJy IMAGR3: 19872 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -664.520 MicroJy iter= 23487 IMAGR3: Field 1 Clean flux density= 531.038 MilliJy 23487 comps IMAGR3: Total Cleaned flux density = 562.745 MilliJy 23893 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.9 MilliJy,max = 1.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 554.18 MicroJy IMAGR3: 19830 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -640.455 MicroJy iter= 26714 IMAGR3: Field 1 Clean flux density= 525.974 MilliJy 26714 comps IMAGR3: Total Cleaned flux density = 557.681 MilliJy 27120 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.8 MilliJy,max = 1.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 537.29 MicroJy IMAGR3: 19791 Residual map points loaded IMAGR3: Field 1 min allowed flux = 619.207 MicroJy iter= 29790 IMAGR3: Field 1 Clean flux density= 515.236 MilliJy 29790 comps IMAGR3: Total Cleaned flux density = 546.943 MilliJy 30196 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 2 min = -1.1 MilliJy,max = 1.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 536.87 MicroJy IMAGR3: 50 Residual map points loaded IMAGR3: Field 2 min algorithm flux= -546.245 MicroJy iter= 434 IMAGR3: Field 2 Clean flux density= 31.764 MilliJy 434 comps IMAGR3: Total Cleaned flux density = 547.000 MilliJy 30224 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.8 MilliJy,max = 1.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 511.86 MicroJy IMAGR3: 19904 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 577.281 MicroJy iter= 33509 IMAGR3: Field 1 Clean flux density= 509.443 MilliJy 33509 comps IMAGR3: Total Cleaned flux density = 541.207 MilliJy 33943 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.8 MilliJy,max = 1.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 500.48 MicroJy IMAGR3: 19889 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -565.510 MicroJy iter= 37291 IMAGR3: Field 1 Clean flux density= 499.500 MilliJy 37291 comps IMAGR3: Total Cleaned flux density = 531.265 MilliJy 37725 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.8 MilliJy,max = 1.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 482.79 MicroJy IMAGR3: 19834 Residual map points loaded IMAGR3: Field 1 min allowed flux = 584.490 MicroJy iter= 38951 IMAGR3: Field 1 Clean flux density= 501.207 MilliJy 38951 comps IMAGR3: Total Cleaned flux density = 532.972 MilliJy 39385 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.7 MilliJy,max = 1.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 460.21 MicroJy IMAGR3: 19797 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -507.129 MicroJy iter= 42739 IMAGR3: Field 1 Clean flux density= 493.365 MilliJy 42739 comps IMAGR3: Total Cleaned flux density = 525.130 MilliJy 43173 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 2 min = -826.2 MicroJy,max = 679.7 MicroJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 459.85 MicroJy IMAGR3: 19 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 465.256 MicroJy iter= 453 IMAGR3: Field 2 Clean flux density= 31.370 MilliJy 453 comps IMAGR3: Total Cleaned flux density = 524.735 MilliJy 43192 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.7 MilliJy,max = 1.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 438.11 MicroJy IMAGR3: 19951 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 484.231 MicroJy iter= 46948 IMAGR3: Field 1 Clean flux density= 490.190 MilliJy 46948 comps IMAGR3: Total Cleaned flux density = 521.561 MilliJy 47401 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.6 MilliJy,max = 1.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 435.21 MicroJy IMAGR3: 19932 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -482.696 MicroJy iter= 51108 IMAGR3: Field 1 Clean flux density= 479.325 MilliJy 51108 comps IMAGR3: Total Cleaned flux density = 510.697 MilliJy 51561 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.7 MilliJy,max = 1.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 433.11 MicroJy IMAGR3: 19916 Residual map points loaded IMAGR3: Field 1 min allowed flux = -578.608 MicroJy iter= 51378 IMAGR3: Field 1 Clean flux density= 478.801 MilliJy 51378 comps IMAGR3: Total Cleaned flux density = 510.173 MilliJy 51831 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.6 MilliJy,max = 1.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 422.81 MicroJy IMAGR3: 19907 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -462.292 MicroJy iter= 56240 IMAGR3: Field 1 Clean flux density= 471.987 MilliJy 56240 comps IMAGR3: Total Cleaned flux density = 503.361 MilliJy 56693 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 2 min = -1.0 MilliJy,max = 1.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 422.87 MicroJy IMAGR3: 94 Residual map points loaded IMAGR3: Field 2 min allowed flux = 536.359 MicroJy iter= 472 IMAGR3: Field 2 Clean flux density= 31.495 MilliJy 472 comps IMAGR3: Total Cleaned flux density = 503.486 MilliJy 56712 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -867.1 MicroJy,max = 657.2 MicroJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 422.77 MicroJy IMAGR3: 49 Residual map points loaded IMAGR3: Field 2 min Clean flux = 441.193 MicroJy iter= 496 IMAGR3: Field 2 Clean flux density= 31.659 MilliJy 496 comps IMAGR3: Total Cleaned flux density = 503.650 MilliJy 56736 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.5 MilliJy,max = 1.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 411.65 MicroJy IMAGR3: 19972 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 453.028 MicroJy iter= 61193 IMAGR3: Field 1 Clean flux density= 457.751 MilliJy 61193 comps IMAGR3: Total Cleaned flux density = 489.415 MilliJy 61689 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Field 1 min = -1.6 MilliJy,max = 1.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 412.70 MicroJy IMAGR3: 19971 Residual map points loaded IMAGR3: Field 1 min allowed flux = 587.432 MicroJy iter= 61319 IMAGR3: Field 1 Clean flux density= 457.746 MilliJy 61319 comps IMAGR3: Total Cleaned flux density = 489.410 MilliJy 61815 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.5 MilliJy,max = 1.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 404.55 MicroJy IMAGR3: 19984 Residual map points loaded IMAGR3: Field 1 min Clean flux = 442.519 MicroJy iter= 66343 IMAGR3: Field 1 Clean flux density= 446.140 MilliJy 66343 comps IMAGR3: Total Cleaned flux density = 477.803 MilliJy 66839 comps IMAGR3: ALGSTB: All 1382 Rows In AP (Max 2059) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 1371- 0 Cells, with 23491 Pts IMAGR3: Peak residual in window 442.519 less than limit 442.520 MicroJy IMAGR3: Merging the Clean components files IMAGR3: Field 1 compressed from 66343 to 21948 components IMAGR3: Field 2 compressed from 496 to 176 components IMAGR3: Field 1 min = -1.5 MilliJy,max = 1.5 MilliJy IMAGR3: Field 2 min = -1.1 MilliJy,max = 1.3 MilliJy IMAGR3: Restoring Clean components IMAGR3: Restoring overlapped Clean components IMAGR3: Restore 617.353 MilliJy ( 253 CCs) from field 1 to field 2 IMAGR3: Restore 31.659 MilliJy ( 176 CCs) from field 2 to field 1 IMAGR3: Checking image max/min IMAGR3: Field 1 final Clean flux 477.799 MilliJy IMAGR3: Field 2 final Clean flux 649.012 MilliJy IMAGR3: Deleting UV work file: IMAGR3: Destroyed 1 extension files of type AN IMAGR3: Destroyed 1 extension files of type FQ IMAGR3: Destroyed UV image file: catno= 7 disk= 1 IMAGR3: Appears to have ended successfully IMAGR3: auto 31DEC06 TST: Cpu= 139.1 Real= 597 TFC@G991216_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 7 disk= 1 AIPS 3: Disk 1 in-CNO 8 renumbered as CNO 6 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.07375 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@0509+101_X,BAND.0-1 >> /home/auto/run/AK485_2000J AIPS 3: AN28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :2 =0509+101' AIPS 3: ' ' AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 8 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 9 disk= 1 AIPS 3: Disk 1 in-CNO 10 renumbered as CNO 7 AIPS 3: Disk 1 in-CNO 11 renumbered as CNO 8 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.126 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0137+331_X,BAND.0-1 >& /dev/null SETFC3: Task SETFC (release of 31DEC06) begins SETFC3: Found 0137+331 X BAND Seq 1 Disk: 1 in slot 5 SETFC3: SETCEL: recommends IMSIZE 1363 CELLSIZE 0.23481 SETFC3: SETCEL: returns IMSIZE 1024 CELLSIZE 0.23481 SETFC3: ZTXOP2: using translated file name = SETFC3: ZTXOP2: /tmp/SETFC@0137+331_X,BAND.0-1 SETFC3: FLYEYE added 7 fields to BOXFILE to 0.056 deg SETFC3: Searching catalog between 0.06 and 0.13 degrees radius SETFC3: ZTXOP2: using translated file name = SETFC3: ZTXOP2: /home/auto/aips/TEXT/STARS/NV00.0030 SETFC3: No NVSS sources selected for BOXFILE SETFC3: The Sun is 87.7 deg away - ignoring SETFC3: First field number written was 1 SETFC3: Highest field number written was 7 SETFC3: returns adverbs to AIPS SETFC3: Appears to have ended successfully SETFC3: auto 31DEC06 TST: Cpu= 0.1 Real= 1 C 1 1012 1012 01 37 41.30 33 09 35.1 00001 -1 507 512 513 C 2 1012 1012 01 37 41.30 33 06 15.2 00002 -1 507 512 513 C 3 1012 1012 01 37 27.52 33 07 55.1 00003 -1 507 512 513 C 4 1012 1012 01 37 55.08 33 07 55.1 00004 -1 507 512 513 C 5 1012 1012 01 37 27.51 33 11 15.0 00005 -1 507 512 513 C 6 1012 1012 01 37 55.09 33 11 15.0 00006 -1 507 512 513 C 7 1012 1012 01 37 41.30 33 12 55.0 00007 -1 507 512 513 TFC@G991216_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 7 disk= 1 AIPS 3: Disk 1 in-CNO 8 renumbered as CNO 6 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.07375 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@0509+101_X,BAND.0-1 >> /home/auto/run/AK485_2000J AIPS 3: AN28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :2 =0509+101' AIPS 3: ' ' AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 8 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 9 disk= 1 AIPS 3: Disk 1 in-CNO 10 renumbered as CNO 7 AIPS 3: Disk 1 in-CNO 11 renumbered as CNO 8 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.126 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0137+331_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@0137+331_X,BAND.0-1 >> /home/auto/run/AK485_2000J AIPS 3: AN28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :3 =0137+331' AIPS 3: ' ' IMAGR3: Task IMAGR (release of 31DEC06) begins IMAGR3: ZTXOP2: using translated file name = IMAGR3: ZTXOP2: /tmp/SETFC@0137+331_X,BAND.0-1 IMAGR3: FIELDF: Final field parameters and # read are: IMAGR3: Field 1 1012 1012 6.2786E-03 -3.4000E-02 0 IMAGR3: Field 2 1012 1012 6.2786E-03 -1.9993E+02 0 IMAGR3: Field 3 1012 1012 -1.7303E+02 -1.0003E+02 0 IMAGR3: Field 4 1012 1012 1.7304E+02 -1.0003E+02 0 IMAGR3: Field 5 1012 1012 -1.7316E+02 9.9866E+01 0 IMAGR3: Field 6 1012 1012 1.7317E+02 9.9866E+01 0 IMAGR3: Field 7 1012 1012 6.2786E-03 1.9987E+02 0 IMAGR3: ZTXOP2: using translated file name = IMAGR3: ZTXOP2: /tmp/SETFC@0137+331_X,BAND.0-1 IMAGR3: WINDF: Number of clean boxes/field read as follows: IMAGR3: Field 01: 1 Field 02: 1 Field 03: 1 Field 04: 1 IMAGR3: Field 05: 1 Field 06: 1 Field 07: 1 IMAGR3: Create 0137+331 .IMAGR . 1 (UV) on disk 1 cno 9 IMAGR3: Beginning channel 1 through 1 with 2 IFs IMAGR3: IMACPY: Copied 8047 visibilities to be imaged IMAGR3: **** WARNING data included out of inner portion of UV plane **** IMAGR3: **** Watch for high-frequency & other poor cleaning effects **** IMAGR3: UVWAIT: begin finding uniform weights IMAGR3: UVWAIT: Average grid weight 5.587E+04 IMAGR3: UVWAIT: Adding temperance S 1.117E+04 IMAGR3: UVWAIT: begin applying uniform or other weights IMAGR3: UVWAIT: Sum of weights in 3.468E+07 and out 4.491E+07 IMAGR3: UVWAIT: Noise is increased by a factor 1.156 due to weighting IMAGR3: UVWAIT: Average summed weight 5.587E+04 over 16094 vis IMAGR3: Create 0137+331 .IBM001. 1 (MA) on disk 1 cno 10 IMAGR3: Create 0137+331 .IBM002. 1 (MA) on disk 1 cno 11 IMAGR3: Create 0137+331 .IBM003. 1 (MA) on disk 1 cno 12 IMAGR3: Create 0137+331 .IBM004. 1 (MA) on disk 1 cno 13 IMAGR3: Create 0137+331 .IBM005. 1 (MA) on disk 1 cno 14 IMAGR3: Create 0137+331 .IBM006. 1 (MA) on disk 1 cno 15 IMAGR3: Create 0137+331 .IBM007. 1 (MA) on disk 1 cno 16 IMAGR3: Create 0137+331 .ICL001. 1 (MA) on disk 1 cno 17 IMAGR3: Create 0137+331 .ICL002. 1 (MA) on disk 1 cno 18 IMAGR3: Create 0137+331 .ICL003. 1 (MA) on disk 1 cno 19 IMAGR3: Create 0137+331 .ICL004. 1 (MA) on disk 1 cno 20 IMAGR3: Create 0137+331 .ICL005. 1 (MA) on disk 1 cno 21 IMAGR3: Create 0137+331 .ICL006. 1 (MA) on disk 1 cno 22 IMAGR3: Create 0137+331 .ICL007. 1 (MA) on disk 1 cno 23 IMAGR3: GRDFLT: X and Y convolution type = SPHEROIDAL IMAGR3: GRDFLT: X and Y parms = 3.0000 1.0000 IMAGR3: GRDFLT: convolution function sampled every 1/100 of a cell IMAGR3: GRDMEM: Ave 2 Channels; 8.435100E+09 to 8.485100E+09 Hz IMAGR3: Field 1 Sum of gridding weights = 4.76800E+08 IMAGR3: Field 1 Beam min = -180.6 MilliJy, max = 1.0 Jy IMAGR3: Field 1 fit FWHM = 1.138 x 0.705 arcsec, PA= 79.1 IMAGR3: Field 2 Sum of gridding weights = 4.76800E+08 IMAGR3: Field 2 Beam min = -180.6 MilliJy, max = 1.0 Jy IMAGR3: Field 2 fit FWHM = 1.138 x 0.705 arcsec, PA= 79.0 IMAGR3: Field 3 Sum of gridding weights = 4.76801E+08 IMAGR3: Field 3 Beam min = -159.2 MilliJy, max = 1.0 Jy IMAGR3: Field 3 fit FWHM = 1.140 x 0.705 arcsec, PA= 79.0 IMAGR3: Field 4 Sum of gridding weights = 4.76799E+08 IMAGR3: Field 4 Beam min = -137.1 MilliJy, max = 1.0 Jy IMAGR3: Field 4 fit FWHM = 1.137 x 0.705 arcsec, PA= 79.1 IMAGR3: Field 5 Sum of gridding weights = 4.76800E+08 IMAGR3: Field 5 Beam min = -159.2 MilliJy, max = 1.0 Jy IMAGR3: Field 5 fit FWHM = 1.139 x 0.705 arcsec, PA= 79.1 IMAGR3: Field 6 Sum of gridding weights = 4.76800E+08 IMAGR3: Field 6 Beam min = -137.2 MilliJy, max = 1.0 Jy IMAGR3: Field 6 fit FWHM = 1.137 x 0.705 arcsec, PA= 79.2 IMAGR3: Field 7 Sum of gridding weights = 4.76800E+08 IMAGR3: Field 7 Beam min = -180.6 MilliJy, max = 1.0 Jy IMAGR3: Field 7 fit FWHM = 1.138 x 0.705 arcsec, PA= 79.1 IMAGR3: CLBHIS: minimum component 0.500 of current peak IMAGR3: Field 1 min = -239.4 MilliJy,max = 2.8 Jy IMAGR3: Field 2 min = -288.4 MilliJy,max = 766.7 MilliJy IMAGR3: Field 3 min = -279.5 MilliJy,max = 1.2 Jy IMAGR3: Field 4 min = -279.5 MilliJy,max = 751.4 MilliJy IMAGR3: Field 5 min = -288.7 MilliJy,max = 752.0 MilliJy IMAGR3: Field 6 min = -290.8 MilliJy,max = 1.2 Jy IMAGR3: Field 7 min = -256.3 MilliJy,max = 769.6 MilliJy IMAGR3: BGC Clean: using 2043 cell beam + residuals > 569.61 MilliJy IMAGR3: 618 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 1.847 Jy iter= 5 IMAGR3: Field 1 Clean flux density= 1.153 Jy 5 comps IMAGR3: Total Cleaned flux density = 1.153 Jy 5 comps IMAGR3: SETDO3: imaging done with multiple tangent planes IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: VISDFT: Model components of type Point IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -146.1 MilliJy,max = 1.7 Jy IMAGR3: BGC Clean: using 2043 cell beam + residuals > 373.72 MilliJy IMAGR3: 471 Residual map points loaded IMAGR3: Field 1 min allowed flux = 795.390 MilliJy iter= 14 IMAGR3: Field 1 Clean flux density= 2.206 Jy 14 comps IMAGR3: Total Cleaned flux density = 2.206 Jy 14 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -77.7 MilliJy,max = 333.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 3.175E-01 < Second best 1.159E+00 IMAGR3: Field 3 min = -79.7 MilliJy,max = 335.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 3.193E-01 < Second best 7.566E-01 IMAGR3: Field 1 min = -75.1 MilliJy,max = 723.6 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 6.883E-01 < Second best 7.337E-01 IMAGR3: Field 7 min = -70.2 MilliJy,max = 222.6 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 2.122E-01 < Second best 7.309E-01 IMAGR3: Field 2 min = -80.9 MilliJy,max = 222.8 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 2.124E-01 < Second best 6.883E-01 IMAGR3: BGC Clean: using 1633 cell beam + residuals > 156.02 MilliJy IMAGR3: 702 Residual map points loaded IMAGR3: Field 1 min allowed flux = 357.432 MilliJy iter= 23 IMAGR3: Field 1 Clean flux density= 2.676 Jy 23 comps IMAGR3: Total Cleaned flux density = 2.676 Jy 23 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -35.7 MilliJy,max = 88.4 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 6.528E-02 < Second best 5.008E-01 IMAGR3: Field 5 min = -35.9 MilliJy,max = 94.6 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 6.388E-02 < Second best 3.400E-01 IMAGR3: Field 1 min = -41.5 MilliJy,max = 325.1 MilliJy IMAGR3: BGC Clean: using 2043 cell beam + residuals > 72.31 MilliJy IMAGR3: 814 Residual map points loaded IMAGR3: Field 1 min allowed flux = 152.006 MilliJy iter= 33 IMAGR3: Field 1 Clean flux density= 2.904 Jy 33 comps IMAGR3: Total Cleaned flux density = 2.904 Jy 33 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -23.4 MilliJy,max = 84.1 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 8.006E-02 < Second best 3.175E-01 IMAGR3: Field 6 min = -22.9 MilliJy,max = 74.7 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 7.111E-02 < Second best 2.124E-01 IMAGR3: Field 2 min = -21.3 MilliJy,max = 56.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 5.387E-02 < Second best 2.122E-01 IMAGR3: Field 7 min = -25.7 MilliJy,max = 70.9 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 6.758E-02 < Second best 1.446E-01 IMAGR3: Field 1 min = -32.0 MilliJy,max = 146.7 MilliJy IMAGR3: BGC Clean: using 2043 cell beam + residuals > 30.75 MilliJy IMAGR3: 1949 Residual map points loaded IMAGR3: Field 1 min allowed flux = 72.680 MilliJy iter= 47 IMAGR3: Field 1 Clean flux density= 3.048 Jy 47 comps IMAGR3: Total Cleaned flux density = 3.048 Jy 47 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -18.1 MilliJy,max = 43.3 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 4.129E-02 < Second best 7.111E-02 IMAGR3: Field 6 min = -16.9 MilliJy,max = 37.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 3.576E-02 < Second best 6.916E-02 IMAGR3: Field 1 min = -27.2 MilliJy,max = 69.8 MilliJy IMAGR3: BGC Clean: using 765 cell beam + residuals > 24.98 MilliJy IMAGR3: 224 Residual map points loaded IMAGR3: Field 1 min allowed flux = 34.804 MilliJy iter= 63 IMAGR3: Field 1 Clean flux density= 3.129 Jy 63 comps IMAGR3: Total Cleaned flux density = 3.129 Jy 63 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -23.0 MilliJy,max = 23.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 2.242E-02 < Second best 6.528E-02 IMAGR3: Field 4 min = -15.1 MilliJy,max = 17.3 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.651E-02 < Second best 6.388E-02 IMAGR3: Field 5 min = -16.6 MilliJy,max = 20.4 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.666E-02 < Second best 5.387E-02 IMAGR3: Field 2 min = -16.1 MilliJy,max = 17.4 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.665E-02 < Second best 4.129E-02 IMAGR3: Field 3 min = -15.6 MilliJy,max = 23.7 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 2.260E-02 < Second best 3.576E-02 IMAGR3: Field 6 min = -13.1 MilliJy,max = 20.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.960E-02 < Second best 3.313E-02 IMAGR3: Field 1 min = -23.1 MilliJy,max = 33.3 MilliJy IMAGR3: BGC Clean: using 1349 cell beam + residuals > 9.08 MilliJy IMAGR3: 4196 Residual map points loaded IMAGR3: Field 1 min allowed flux = 16.551 MilliJy iter= 94 IMAGR3: Field 1 Clean flux density= 3.153 Jy 94 comps IMAGR3: Total Cleaned flux density = 3.153 Jy 94 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -16.7 MilliJy,max = 16.3 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.592E-02 < Second best 2.242E-02 IMAGR3: Field 7 min = -19.7 MilliJy,max = 16.1 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.566E-02 < Second best 1.960E-02 IMAGR3: Field 6 min = -12.9 MilliJy,max = 14.9 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.425E-02 < Second best 1.666E-02 IMAGR3: Field 5 min = -17.0 MilliJy,max = 16.1 MilliJy IMAGR3: BGC Clean: using 1349 cell beam + residuals > 8.70 MilliJy IMAGR3: 2072 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -11.662 MilliJy iter= 38 IMAGR3: Field 5 Clean flux density= 7.454 MilliJy 38 comps IMAGR3: Total Cleaned flux density = 3.161 Jy 132 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -15.9 MilliJy,max = 15.9 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.516E-02 < Second best 1.651E-02 IMAGR3: Field 4 min = -13.8 MilliJy,max = 15.9 MilliJy IMAGR3: BGC Clean: using 1497 cell beam + residuals > 8.40 MilliJy IMAGR3: 2033 Residual map points loaded IMAGR3: Field 4 min algorithm flux= -10.865 MilliJy iter= 44 IMAGR3: Field 4 Clean flux density= 3.484 MilliJy 44 comps IMAGR3: Total Cleaned flux density = 3.164 Jy 176 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -14.0 MilliJy,max = 15.2 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.454E-02 < Second best 1.577E-02 IMAGR3: Field 1 min = -16.6 MilliJy,max = 15.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 7.84 MilliJy IMAGR3: 1524 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 11.047 MilliJy iter= 179 IMAGR3: Field 1 Clean flux density= 3.144 Jy 179 comps IMAGR3: Total Cleaned flux density = 3.155 Jy 261 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -14.1 MilliJy,max = 13.2 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.351E-02 < Second best 1.516E-02 IMAGR3: Field 2 min = -13.6 MilliJy,max = 14.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.352E-02 < Second best 1.454E-02 IMAGR3: Field 3 min = -13.2 MilliJy,max = 13.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.284E-02 < Second best 1.425E-02 IMAGR3: Field 6 min = -12.7 MilliJy,max = 13.4 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 1.281E-02 < Second best 1.352E-02 IMAGR3: BGC Clean: using 103 cell beam + residuals > 7.56 MilliJy IMAGR3: 1486 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 9.995 MilliJy iter= 94 IMAGR3: Field 2 Clean flux density= 28.019 MilliJy 94 comps IMAGR3: Total Cleaned flux density = 3.183 Jy 355 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -14.1 MilliJy,max = 12.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 7.56 MilliJy IMAGR3: 1384 Residual map points loaded IMAGR3: Field 7 min algorithm flux= -9.762 MilliJy iter= 114 IMAGR3: Field 7 Clean flux density= -54.632 MilliJy 114 comps IMAGR3: Total Cleaned flux density = 3.128 Jy 469 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -12.2 MilliJy,max = 12.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 7.51 MilliJy IMAGR3: 1253 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -9.189 MilliJy iter= 111 IMAGR3: Field 3 Clean flux density= -2.975 MilliJy 111 comps IMAGR3: Total Cleaned flux density = 3.125 Jy 580 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -12.6 MilliJy,max = 12.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 7.46 MilliJy IMAGR3: 1177 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -9.004 MilliJy iter= 125 IMAGR3: Field 6 Clean flux density= 54.994 MilliJy 125 comps IMAGR3: Total Cleaned flux density = 3.180 Jy 705 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -11.2 MilliJy,max = 11.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 9.489E-03 < Second best 1.055E-02 IMAGR3: Field 1 min = -8.7 MilliJy,max = 8.2 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 8.202E-03 < Second best 1.039E-02 IMAGR3: Field 4 min = -10.6 MilliJy,max = 11.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 6.41 MilliJy IMAGR3: 1722 Residual map points loaded IMAGR3: Field 4 min algorithm flux= -7.652 MilliJy iter= 187 IMAGR3: Field 4 Clean flux density= -857.657 MicroJy 187 comps IMAGR3: Total Cleaned flux density = 3.176 Jy 848 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -9.2 MilliJy,max = 8.1 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 7.341E-03 < Second best 9.489E-03 IMAGR3: Field 5 min = -11.2 MilliJy,max = 11.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 6.21 MilliJy IMAGR3: 2741 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -7.623 MilliJy iter= 244 IMAGR3: Field 5 Clean flux density= 33.678 MilliJy 244 comps IMAGR3: Total Cleaned flux density = 3.202 Jy 1054 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -8.7 MilliJy,max = 8.6 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 7.222E-03 < Second best 8.786E-03 IMAGR3: Field 3 min = -8.6 MilliJy,max = 8.6 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 7.715E-03 < Second best 8.610E-03 IMAGR3: Field 6 min = -8.8 MilliJy,max = 9.2 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 7.532E-03 < Second best 8.202E-03 IMAGR3: Field 1 min = -8.8 MilliJy,max = 7.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 5.37 MilliJy IMAGR3: 620 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -6.029 MilliJy iter= 305 IMAGR3: Field 1 Clean flux density= 3.144 Jy 305 comps IMAGR3: Total Cleaned flux density = 3.202 Jy 1180 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -8.4 MilliJy,max = 8.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 5.36 MilliJy IMAGR3: 751 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -5.937 MilliJy iter= 241 IMAGR3: Field 3 Clean flux density= 8.198 MilliJy 241 comps IMAGR3: Total Cleaned flux density = 3.213 Jy 1310 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -8.7 MilliJy,max = 8.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 5.35 MilliJy IMAGR3: 643 Residual map points loaded IMAGR3: Field 6 min algorithm flux= 5.829 MilliJy iter= 243 IMAGR3: Field 6 Clean flux density= 46.928 MilliJy 243 comps IMAGR3: Total Cleaned flux density = 3.205 Jy 1428 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -8.7 MilliJy,max = 7.7 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 6.494E-03 < Second best 7.332E-03 IMAGR3: Field 4 min = -8.9 MilliJy,max = 7.7 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 6.810E-03 < Second best 7.304E-03 IMAGR3: Field 5 min = -7.6 MilliJy,max = 7.8 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 6.468E-03 < Second best 7.222E-03 IMAGR3: Field 7 min = -7.8 MilliJy,max = 7.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 4.44 MilliJy IMAGR3: 1107 Residual map points loaded IMAGR3: Field 7 min algorithm flux= -5.053 MilliJy iter= 310 IMAGR3: Field 7 Clean flux density= -42.550 MilliJy 310 comps IMAGR3: Total Cleaned flux density = 3.217 Jy 1624 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -9.1 MilliJy,max = 7.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 4.43 MilliJy IMAGR3: 3526 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 5.283 MilliJy iter= 509 IMAGR3: Field 4 Clean flux density= -13.658 MilliJy 509 comps IMAGR3: Total Cleaned flux density = 3.204 Jy 1946 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -6.1 MilliJy,max = 6.3 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 5.875E-03 < Second best 6.468E-03 IMAGR3: Field 5 min = -7.7 MilliJy,max = 8.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 4.36 MilliJy IMAGR3: 1268 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -4.841 MilliJy iter= 463 IMAGR3: Field 5 Clean flux density= 14.188 MilliJy 463 comps IMAGR3: Total Cleaned flux density = 3.185 Jy 2165 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -6.2 MilliJy,max = 6.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 4.36 MilliJy IMAGR3: 257 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 4.562 MilliJy iter= 194 IMAGR3: Field 2 Clean flux density= 29.564 MilliJy 194 comps IMAGR3: Total Cleaned flux density = 3.186 Jy 2265 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -5.7 MilliJy,max = 5.3 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 5.281E-03 < Second best 5.687E-03 IMAGR3: Field 3 min = -6.2 MilliJy,max = 7.3 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 4.08 MilliJy IMAGR3: 351 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -4.281 MilliJy iter= 346 IMAGR3: Field 3 Clean flux density= 7.347 MilliJy 346 comps IMAGR3: Total Cleaned flux density = 3.185 Jy 2370 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -6.3 MilliJy,max = 6.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 3.87 MilliJy IMAGR3: 597 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -4.124 MilliJy iter= 394 IMAGR3: Field 6 Clean flux density= 51.004 MilliJy 394 comps IMAGR3: Total Cleaned flux density = 3.190 Jy 2521 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -5.7 MilliJy,max = 5.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 3.87 MilliJy IMAGR3: 252 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 4.015 MilliJy iter= 401 IMAGR3: Field 1 Clean flux density= 3.152 Jy 401 comps IMAGR3: Total Cleaned flux density = 3.197 Jy 2617 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -6.5 MilliJy,max = 5.6 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 4.441E-03 < Second best 4.836E-03 IMAGR3: Field 7 min = -6.3 MilliJy,max = 5.6 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 4.194E-03 < Second best 4.639E-03 IMAGR3: Field 5 min = -6.5 MilliJy,max = 6.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 3.20 MilliJy IMAGR3: 2537 Residual map points loaded IMAGR3: Field 5 min algorithm flux= 3.600 MilliJy iter= 798 IMAGR3: Field 5 Clean flux density= 8.893 MilliJy 798 comps IMAGR3: Total Cleaned flux density = 3.192 Jy 2952 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -6.5 MilliJy,max = 6.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 3.20 MilliJy IMAGR3: 1947 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 3.536 MilliJy iter= 818 IMAGR3: Field 4 Clean flux density= 2.228 MilliJy 818 comps IMAGR3: Total Cleaned flux density = 3.208 Jy 3261 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -5.3 MilliJy,max = 4.7 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 3.762E-03 < Second best 4.194E-03 IMAGR3: Field 7 min = -5.3 MilliJy,max = 4.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 3.11 MilliJy IMAGR3: 179 Residual map points loaded IMAGR3: Field 7 min algorithm flux= -3.207 MilliJy iter= 405 IMAGR3: Field 7 Clean flux density= -32.218 MilliJy 405 comps IMAGR3: Total Cleaned flux density = 3.218 Jy 3356 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -5.6 MilliJy,max = 5.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 3.00 MilliJy IMAGR3: 748 Residual map points loaded IMAGR3: Field 3 min algorithm flux= 3.188 MilliJy iter= 550 IMAGR3: Field 3 Clean flux density= 5.112 MilliJy 550 comps IMAGR3: Total Cleaned flux density = 3.216 Jy 3560 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -4.9 MilliJy,max = 4.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.88 MilliJy IMAGR3: 767 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -3.042 MilliJy iter= 593 IMAGR3: Field 6 Clean flux density= 38.584 MilliJy 593 comps IMAGR3: Total Cleaned flux density = 3.204 Jy 3759 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -4.2 MilliJy,max = 3.9 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 3.419E-03 < Second best 3.762E-03 IMAGR3: Field 2 min = -5.1 MilliJy,max = 4.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.79 MilliJy IMAGR3: 596 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 2.936 MilliJy iter= 386 IMAGR3: Field 2 Clean flux density= 24.043 MilliJy 386 comps IMAGR3: Total Cleaned flux density = 3.198 Jy 3951 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -5.2 MilliJy,max = 5.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.64 MilliJy IMAGR3: 1233 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -2.821 MilliJy iter= 1076 IMAGR3: Field 5 Clean flux density= 7.957 MilliJy 1076 comps IMAGR3: Total Cleaned flux density = 3.197 Jy 4229 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -3.9 MilliJy,max = 3.5 MilliJy IMAGR3: TRY ANOTHER FIELD: this is 3.198E-03 < Second best 3.390E-03 IMAGR3: Field 4 min = -5.4 MilliJy,max = 5.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.45 MilliJy IMAGR3: 1297 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 2.621 MilliJy iter= 1116 IMAGR3: Field 4 Clean flux density= 12.773 MilliJy 1116 comps IMAGR3: Total Cleaned flux density = 3.208 Jy 4527 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -3.8 MilliJy,max = 3.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.44 MilliJy IMAGR3: 907 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 2.587 MilliJy iter= 659 IMAGR3: Field 1 Clean flux density= 3.142 Jy 659 comps IMAGR3: Total Cleaned flux density = 3.198 Jy 4785 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -4.3 MilliJy,max = 3.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.40 MilliJy IMAGR3: 213 Residual map points loaded IMAGR3: Field 7 min algorithm flux= 2.458 MilliJy iter= 504 IMAGR3: Field 7 Clean flux density= -29.450 MilliJy 504 comps IMAGR3: Total Cleaned flux density = 3.201 Jy 4884 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -4.2 MilliJy,max = 5.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.32 MilliJy IMAGR3: 886 Residual map points loaded IMAGR3: Field 3 min algorithm flux= 2.436 MilliJy iter= 788 IMAGR3: Field 3 Clean flux density= 4.433 MilliJy 788 comps IMAGR3: Total Cleaned flux density = 3.200 Jy 5122 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -4.1 MilliJy,max = 4.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.23 MilliJy IMAGR3: 1346 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -2.370 MilliJy iter= 907 IMAGR3: Field 6 Clean flux density= 47.127 MilliJy 907 comps IMAGR3: Total Cleaned flux density = 3.209 Jy 5436 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -4.0 MilliJy,max = 3.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.16 MilliJy IMAGR3: 328 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 2.217 MilliJy iter= 524 IMAGR3: Field 2 Clean flux density= 21.278 MilliJy 524 comps IMAGR3: Total Cleaned flux density = 3.206 Jy 5574 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -4.6 MilliJy,max = 4.3 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 2.06 MilliJy IMAGR3: 1311 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -2.185 MilliJy iter= 1403 IMAGR3: Field 5 Clean flux density= 1.679 MilliJy 1403 comps IMAGR3: Total Cleaned flux density = 3.200 Jy 5901 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -4.6 MilliJy,max = 4.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.99 MilliJy IMAGR3: 1332 Residual map points loaded IMAGR3: Field 4 min algorithm flux= -2.101 MilliJy iter= 1445 IMAGR3: Field 4 Clean flux density= 16.653 MilliJy 1445 comps IMAGR3: Total Cleaned flux density = 3.203 Jy 6230 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -3.3 MilliJy,max = 2.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.92 MilliJy IMAGR3: 894 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -1.999 MilliJy iter= 913 IMAGR3: Field 1 Clean flux density= 3.142 Jy 913 comps IMAGR3: Total Cleaned flux density = 3.204 Jy 6484 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -3.8 MilliJy,max = 3.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.89 MilliJy IMAGR3: 295 Residual map points loaded IMAGR3: Field 7 min algorithm flux= -1.930 MilliJy iter= 638 IMAGR3: Field 7 Clean flux density= -27.885 MilliJy 638 comps IMAGR3: Total Cleaned flux density = 3.205 Jy 6618 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -3.5 MilliJy,max = 4.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.83 MilliJy IMAGR3: 1113 Residual map points loaded IMAGR3: Field 3 min algorithm flux= 1.921 MilliJy iter= 1078 IMAGR3: Field 3 Clean flux density= 13.341 MilliJy 1078 comps IMAGR3: Total Cleaned flux density = 3.214 Jy 6908 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -3.5 MilliJy,max = 3.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.75 MilliJy IMAGR3: 1211 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -1.836 MilliJy iter= 1223 IMAGR3: Field 6 Clean flux density= 48.472 MilliJy 1223 comps IMAGR3: Total Cleaned flux density = 3.216 Jy 7224 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -3.1 MilliJy,max = 3.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.72 MilliJy IMAGR3: 386 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 1.762 MilliJy iter= 692 IMAGR3: Field 2 Clean flux density= 22.503 MilliJy 692 comps IMAGR3: Total Cleaned flux density = 3.217 Jy 7392 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -3.8 MilliJy,max = 3.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.65 MilliJy IMAGR3: 1532 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -1.743 MilliJy iter= 1783 IMAGR3: Field 5 Clean flux density= 6.656 MilliJy 1783 comps IMAGR3: Total Cleaned flux density = 3.222 Jy 7772 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -4.1 MilliJy,max = 3.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.59 MilliJy IMAGR3: 1516 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 1.675 MilliJy iter= 1828 IMAGR3: Field 4 Clean flux density= 16.532 MilliJy 1828 comps IMAGR3: Total Cleaned flux density = 3.222 Jy 8155 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -2.5 MilliJy,max = 2.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.54 MilliJy IMAGR3: 921 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -1.600 MilliJy iter= 1192 IMAGR3: Field 1 Clean flux density= 3.142 Jy 1192 comps IMAGR3: Total Cleaned flux density = 3.221 Jy 8434 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -3.3 MilliJy,max = 2.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.52 MilliJy IMAGR3: 425 Residual map points loaded IMAGR3: Field 7 min algorithm flux= -1.556 MilliJy iter= 805 IMAGR3: Field 7 Clean flux density= -29.770 MilliJy 805 comps IMAGR3: Total Cleaned flux density = 3.220 Jy 8601 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -2.8 MilliJy,max = 3.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.48 MilliJy IMAGR3: 1673 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -1.553 MilliJy iter= 1487 IMAGR3: Field 3 Clean flux density= 12.968 MilliJy 1487 comps IMAGR3: Total Cleaned flux density = 3.219 Jy 9010 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -3.0 MilliJy,max = 3.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.43 MilliJy IMAGR3: 1694 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -1.505 MilliJy iter= 1640 IMAGR3: Field 6 Clean flux density= 49.741 MilliJy 1640 comps IMAGR3: Total Cleaned flux density = 3.220 Jy 9427 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -2.5 MilliJy,max = 3.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.41 MilliJy IMAGR3: 786 Residual map points loaded IMAGR3: Field 2 min algorithm flux= -1.461 MilliJy iter= 974 IMAGR3: Field 2 Clean flux density= 18.488 MilliJy 974 comps IMAGR3: Total Cleaned flux density = 3.216 Jy 9709 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -3.3 MilliJy,max = 3.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.37 MilliJy IMAGR3: 2067 Residual map points loaded IMAGR3: Field 5 min algorithm flux= 1.451 MilliJy iter= 2254 IMAGR3: Field 5 Clean flux density= 5.835 MilliJy 2254 comps IMAGR3: Total Cleaned flux density = 3.216 Jy 10180 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -3.3 MilliJy,max = 3.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.33 MilliJy IMAGR3: 1702 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 1.393 MilliJy iter= 2268 IMAGR3: Field 4 Clean flux density= 18.450 MilliJy 2268 comps IMAGR3: Total Cleaned flux density = 3.218 Jy 10620 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.9 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.31 MilliJy IMAGR3: 1731 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 1.365 MilliJy iter= 1619 IMAGR3: Field 1 Clean flux density= 3.151 Jy 1619 comps IMAGR3: Total Cleaned flux density = 3.226 Jy 11047 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -2.8 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.30 MilliJy IMAGR3: 736 Residual map points loaded IMAGR3: Field 7 min algorithm flux= -1.330 MilliJy iter= 1059 IMAGR3: Field 7 Clean flux density= -30.955 MilliJy 1059 comps IMAGR3: Total Cleaned flux density = 3.225 Jy 11301 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -2.5 MilliJy,max = 3.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.27 MilliJy IMAGR3: 2009 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -1.329 MilliJy iter= 1991 IMAGR3: Field 3 Clean flux density= 3.034 MilliJy 1991 comps IMAGR3: Total Cleaned flux density = 3.215 Jy 11805 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -2.7 MilliJy,max = 2.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.24 MilliJy IMAGR3: 1958 Residual map points loaded IMAGR3: Field 6 min algorithm flux= 1.297 MilliJy iter= 2152 IMAGR3: Field 6 Clean flux density= 53.950 MilliJy 2152 comps IMAGR3: Total Cleaned flux density = 3.219 Jy 12317 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -2.2 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.22 MilliJy IMAGR3: 695 Residual map points loaded IMAGR3: Field 2 min algorithm flux= -1.251 MilliJy iter= 1239 IMAGR3: Field 2 Clean flux density= 17.785 MilliJy 1239 comps IMAGR3: Total Cleaned flux density = 3.219 Jy 12582 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -2.7 MilliJy,max = 3.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.19 MilliJy IMAGR3: 1727 Residual map points loaded IMAGR3: Field 5 min algorithm flux= 1.243 MilliJy iter= 2699 IMAGR3: Field 5 Clean flux density= 14.117 MilliJy 2699 comps IMAGR3: Total Cleaned flux density = 3.227 Jy 13027 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -3.0 MilliJy,max = 3.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.16 MilliJy IMAGR3: 1664 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 1.212 MilliJy iter= 2692 IMAGR3: Field 4 Clean flux density= 17.570 MilliJy 2692 comps IMAGR3: Total Cleaned flux density = 3.226 Jy 13451 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.7 MilliJy,max = 1.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.13 MilliJy IMAGR3: 998 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -1.158 MilliJy iter= 1922 IMAGR3: Field 1 Clean flux density= 3.147 Jy 1922 comps IMAGR3: Total Cleaned flux density = 3.223 Jy 13754 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -2.2 MilliJy,max = 2.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.10 MilliJy IMAGR3: 1078 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -1.130 MilliJy iter= 2345 IMAGR3: Field 3 Clean flux density= 6.838 MilliJy 2345 comps IMAGR3: Total Cleaned flux density = 3.226 Jy 14108 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -2.6 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.08 MilliJy IMAGR3: 703 Residual map points loaded IMAGR3: Field 7 min algorithm flux= -1.105 MilliJy iter= 1329 IMAGR3: Field 7 Clean flux density= -27.176 MilliJy 1329 comps IMAGR3: Total Cleaned flux density = 3.230 Jy 14378 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -2.4 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.05 MilliJy IMAGR3: 1840 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -1.087 MilliJy iter= 2636 IMAGR3: Field 6 Clean flux density= 52.186 MilliJy 2636 comps IMAGR3: Total Cleaned flux density = 3.228 Jy 14862 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -1.9 MilliJy,max = 2.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.03 MilliJy IMAGR3: 1003 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 1.060 MilliJy iter= 1583 IMAGR3: Field 2 Clean flux density= 18.621 MilliJy 1583 comps IMAGR3: Total Cleaned flux density = 3.229 Jy 15206 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -2.7 MilliJy,max = 2.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 1.01 MilliJy IMAGR3: 2821 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -1.063 MilliJy iter= 3344 IMAGR3: Field 5 Clean flux density= 10.616 MilliJy 3344 comps IMAGR3: Total Cleaned flux density = 3.226 Jy 15851 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -2.6 MilliJy,max = 2.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 988.29 MicroJy IMAGR3: 2244 Residual map points loaded IMAGR3: Field 4 min algorithm flux= -1.030 MilliJy iter= 3312 IMAGR3: Field 4 Clean flux density= 18.645 MilliJy 3312 comps IMAGR3: Total Cleaned flux density = 3.227 Jy 16471 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.6 MilliJy,max = 1.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 976.33 MicroJy IMAGR3: 2563 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -1.022 MilliJy iter= 2491 IMAGR3: Field 1 Clean flux density= 3.148 Jy 2491 comps IMAGR3: Total Cleaned flux density = 3.228 Jy 17040 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -2.3 MilliJy,max = 2.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 976.13 MicroJy IMAGR3: 3776 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -1.035 MilliJy iter= 3138 IMAGR3: Field 3 Clean flux density= -58.352 MicroJy 3138 comps IMAGR3: Total Cleaned flux density = 3.221 Jy 17833 comps IMAGR3: ALGSTB: All 471 Rows In AP (Max 1035) IMAGR3: ALGSTB field 3 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 460- 0 Cells, with 8047 Pts IMAGR3: Field 7 min = -2.4 MilliJy,max = 1.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 974.04 MicroJy IMAGR3: 1747 Residual map points loaded IMAGR3: Field 7 min algorithm flux= 1.012 MilliJy iter= 1832 IMAGR3: Field 7 Clean flux density= -29.703 MilliJy 1832 comps IMAGR3: Total Cleaned flux density = 3.218 Jy 18336 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -2.4 MilliJy,max = 2.3 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 968.29 MicroJy IMAGR3: 2673 Residual map points loaded IMAGR3: Field 6 min algorithm flux= 1.016 MilliJy iter= 3293 IMAGR3: Field 6 Clean flux density= 61.390 MilliJy 3293 comps IMAGR3: Total Cleaned flux density = 3.228 Jy 18993 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -2.4 MilliJy,max = 2.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 957.24 MicroJy IMAGR3: 2231 Residual map points loaded IMAGR3: Field 5 min algorithm flux= 1.003 MilliJy iter= 3935 IMAGR3: Field 5 Clean flux density= 5.740 MilliJy 3935 comps IMAGR3: Total Cleaned flux density = 3.223 Jy 19584 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -1.8 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 953.05 MicroJy IMAGR3: 1573 Residual map points loaded IMAGR3: Field 2 min algorithm flux= -986.266 MicroJy iter= 2062 IMAGR3: Field 2 Clean flux density= 9.870 MilliJy 2062 comps IMAGR3: Total Cleaned flux density = 3.214 Jy 20063 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -1.8 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 928.83 MicroJy IMAGR3: 547 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -942.553 MicroJy iter= 3359 IMAGR3: Field 3 Clean flux density= 719.332 MicroJy 3359 comps IMAGR3: Total Cleaned flux density = 3.215 Jy 20284 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -2.6 MilliJy,max = 2.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 917.83 MicroJy IMAGR3: 2169 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 954.637 MicroJy iter= 3889 IMAGR3: Field 4 Clean flux density= 26.209 MilliJy 3889 comps IMAGR3: Total Cleaned flux density = 3.222 Jy 20861 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.5 MilliJy,max = 1.4 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 899.99 MicroJy IMAGR3: 1967 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 931.362 MicroJy iter= 2972 IMAGR3: Field 1 Clean flux density= 3.139 Jy 2972 comps IMAGR3: Total Cleaned flux density = 3.213 Jy 21342 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -2.3 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 886.78 MicroJy IMAGR3: 2789 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -925.077 MicroJy iter= 3940 IMAGR3: Field 6 Clean flux density= 65.891 MilliJy 3940 comps IMAGR3: Total Cleaned flux density = 3.218 Jy 21989 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -2.1 MilliJy,max = 1.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 867.30 MicroJy IMAGR3: 562 Residual map points loaded IMAGR3: Field 7 min algorithm flux= 879.871 MicroJy iter= 2060 IMAGR3: Field 7 Clean flux density= -26.891 MilliJy 2060 comps IMAGR3: Total Cleaned flux density = 3.221 Jy 22217 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -2.4 MilliJy,max = 2.3 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 850.56 MicroJy IMAGR3: 2372 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -885.267 MicroJy iter= 4535 IMAGR3: Field 5 Clean flux density= 6.142 MilliJy 4535 comps IMAGR3: Total Cleaned flux density = 3.221 Jy 22817 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -1.5 MilliJy,max = 1.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 835.92 MicroJy IMAGR3: 1853 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 865.186 MicroJy iter= 2565 IMAGR3: Field 2 Clean flux density= 10.694 MilliJy 2565 comps IMAGR3: Total Cleaned flux density = 3.222 Jy 23320 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -2.5 MilliJy,max = 2.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 820.27 MicroJy IMAGR3: 1913 Residual map points loaded IMAGR3: Field 4 min algorithm flux= -851.294 MicroJy iter= 4416 IMAGR3: Field 4 Clean flux density= 24.495 MilliJy 4416 comps IMAGR3: Total Cleaned flux density = 3.220 Jy 23847 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -1.8 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 821.00 MicroJy IMAGR3: 2246 Residual map points loaded IMAGR3: SOMETHING IS GOING WRONG - ABANDON CLEAN IMAGR3: Field 3 min algorithm flux= -1.246 MilliJy iter= 3363 IMAGR3: Field 3 Clean flux density= 728.537 MicroJy 3363 comps IMAGR3: Total Cleaned flux density = 3.220 Jy 23851 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -1.8 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 820.45 MicroJy IMAGR3: 2155 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -845.366 MicroJy iter= 3979 IMAGR3: Field 3 Clean flux density= 5.737 MilliJy 3979 comps IMAGR3: Total Cleaned flux density = 3.225 Jy 24467 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.5 MilliJy,max = 1.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 804.34 MicroJy IMAGR3: 1794 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 833.300 MicroJy iter= 3445 IMAGR3: Field 1 Clean flux density= 3.136 Jy 3445 comps IMAGR3: Total Cleaned flux density = 3.222 Jy 24940 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -2.1 MilliJy,max = 2.3 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 790.35 MicroJy IMAGR3: 3399 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -828.865 MicroJy iter= 4705 IMAGR3: Field 6 Clean flux density= 73.660 MilliJy 4705 comps IMAGR3: Total Cleaned flux density = 3.230 Jy 25705 comps IMAGR3: ALGSTB: All 471 Rows In AP (Max 1035) IMAGR3: ALGSTB field 6 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 460- 0 Cells, with 8047 Pts IMAGR3: Field 5 min = -2.3 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 788.77 MicroJy IMAGR3: 3956 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -825.931 MicroJy iter= 5419 IMAGR3: Field 5 Clean flux density= 453.735 MicroJy 5419 comps IMAGR3: Total Cleaned flux density = 3.224 Jy 26589 comps IMAGR3: ALGSTB: All 471 Rows In AP (Max 1035) IMAGR3: ALGSTB field 5 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 460- 0 Cells, with 8047 Pts IMAGR3: Field 7 min = -1.8 MilliJy,max = 1.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 790.98 MicroJy IMAGR3: 1974 Residual map points loaded IMAGR3: Field 7 min algorithm flux= 821.225 MicroJy iter= 2581 IMAGR3: Field 7 Clean flux density= -19.173 MilliJy 2581 comps IMAGR3: Total Cleaned flux density = 3.232 Jy 27110 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -1.5 MilliJy,max = 1.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 785.25 MicroJy IMAGR3: 1971 Residual map points loaded IMAGR3: Field 2 min algorithm flux= 811.381 MicroJy iter= 3090 IMAGR3: Field 2 Clean flux density= 5.865 MilliJy 3090 comps IMAGR3: Total Cleaned flux density = 3.227 Jy 27635 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -2.2 MilliJy,max = 2.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 782.43 MicroJy IMAGR3: 2294 Residual map points loaded IMAGR3: Field 4 min algorithm flux= 810.521 MicroJy iter= 5030 IMAGR3: Field 4 Clean flux density= 20.691 MilliJy 5030 comps IMAGR3: Total Cleaned flux density = 3.223 Jy 28249 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -1.9 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 788.76 MicroJy IMAGR3: 4291 Residual map points loaded IMAGR3: SOMETHING IS GOING WRONG - ABANDON CLEAN IMAGR3: Field 3 min algorithm flux= -1.241 MilliJy iter= 3990 IMAGR3: Field 3 Clean flux density= 4.551 MilliJy 3990 comps IMAGR3: Total Cleaned flux density = 3.222 Jy 28260 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -1.8 MilliJy,max = 2.1 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 785.90 MicroJy IMAGR3: 3851 Residual map points loaded IMAGR3: Field 3 min algorithm flux= -821.087 MicroJy iter= 4931 IMAGR3: Field 3 Clean flux density= 13.166 MilliJy 4931 comps IMAGR3: Total Cleaned flux density = 3.231 Jy 29201 comps IMAGR3: ALGSTB: All 471 Rows In AP (Max 1035) IMAGR3: ALGSTB field 3 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 460- 0 Cells, with 8047 Pts IMAGR3: Field 1 min = -1.6 MilliJy,max = 1.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 794.83 MicroJy IMAGR3: 3848 Residual map points loaded IMAGR3: Field 1 min algorithm flux= -833.638 MicroJy iter= 4294 IMAGR3: Field 1 Clean flux density= 3.122 Jy 4294 comps IMAGR3: Total Cleaned flux density = 3.217 Jy 30050 comps IMAGR3: ALGSTB: All 471 Rows In AP (Max 1035) IMAGR3: ALGSTB field 1 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 460- 0 Cells, with 8047 Pts IMAGR3: Field 1 min = -1.2 MilliJy,max = 1.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 777.75 MicroJy IMAGR3: 723 Residual map points loaded IMAGR3: Field 1 min allowed flux = 824.447 MicroJy iter= 4461 IMAGR3: Field 1 Clean flux density= 3.136 Jy 4461 comps IMAGR3: Total Cleaned flux density = 3.231 Jy 30217 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -2.1 MilliJy,max = 1.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 775.84 MicroJy IMAGR3: 3499 Residual map points loaded IMAGR3: Field 6 min algorithm flux= -808.380 MicroJy iter= 5511 IMAGR3: Field 6 Clean flux density= 57.236 MilliJy 5511 comps IMAGR3: Total Cleaned flux density = 3.214 Jy 31023 comps IMAGR3: ALGSTB: All 471 Rows In AP (Max 1035) IMAGR3: ALGSTB field 6 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 460- 0 Cells, with 8047 Pts IMAGR3: Field 5 min = -2.2 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 770.50 MicroJy IMAGR3: 3633 Residual map points loaded IMAGR3: SOMETHING IS GOING WRONG - ABANDON CLEAN IMAGR3: Field 5 min algorithm flux= -1.144 MilliJy iter= 5443 IMAGR3: Field 5 Clean flux density= 1.485 MilliJy 5443 comps IMAGR3: Total Cleaned flux density = 3.215 Jy 31047 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -2.2 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 767.78 MicroJy IMAGR3: 3130 Residual map points loaded IMAGR3: Field 5 min algorithm flux= -794.549 MicroJy iter= 6231 IMAGR3: Field 5 Clean flux density= 9.399 MilliJy 6231 comps IMAGR3: Total Cleaned flux density = 3.223 Jy 31835 comps IMAGR3: ALGSTB: All 471 Rows In AP (Max 1035) IMAGR3: ALGSTB field 5 Ipol gridded model subtraction chns 1- 2 IMAGR3: ALGSTB: Pass 1; 460- 0 Cells, with 8047 Pts IMAGR3: Field 1 min = -1.2 MilliJy,max = 1.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 768.24 MicroJy IMAGR3: 898 Residual map points loaded IMAGR3: Field 1 min algorithm flux= 782.821 MicroJy iter= 4715 IMAGR3: Field 1 Clean flux density= 3.138 Jy 4715 comps IMAGR3: Total Cleaned flux density = 3.226 Jy 32089 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -1.7 MilliJy,max = 1.8 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 753.02 MicroJy IMAGR3: 1984 Residual map points loaded IMAGR3: Field 3 min algorithm flux= 775.951 MicroJy iter= 5437 IMAGR3: Field 3 Clean flux density= 11.696 MilliJy 5437 comps IMAGR3: Total Cleaned flux density = 3.224 Jy 32595 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -1.4 MilliJy,max = 1.3 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 743.12 MicroJy IMAGR3: 1061 Residual map points loaded IMAGR3: Field 7 min algorithm flux= 760.484 MicroJy iter= 2911 IMAGR3: Field 7 Clean flux density= -17.567 MilliJy 2911 comps IMAGR3: Total Cleaned flux density = 3.226 Jy 32925 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 2 min = -1.5 MilliJy,max = 1.5 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 732.90 MicroJy IMAGR3: 1149 Residual map points loaded IMAGR3: Field 2 min Clean flux = -755.663 MicroJy iter= 3422 IMAGR3: Field 2 Clean flux density= 4.102 MilliJy 3422 comps IMAGR3: Total Cleaned flux density = 3.224 Jy 33257 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 4 min = -2.4 MilliJy,max = 2.0 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 717.27 MicroJy IMAGR3: 2405 Residual map points loaded IMAGR3: Field 4 min Clean flux = -755.888 MicroJy iter= 5575 IMAGR3: Field 4 Clean flux density= 22.293 MilliJy 5575 comps IMAGR3: Total Cleaned flux density = 3.226 Jy 33802 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 6 min = -1.5 MilliJy,max = 1.7 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 674.75 MicroJy IMAGR3: 1756 Residual map points loaded IMAGR3: Field 6 min Clean flux = -754.818 MicroJy iter= 5738 IMAGR3: Field 6 Clean flux density= 54.677 MilliJy 5738 comps IMAGR3: Total Cleaned flux density = 3.223 Jy 34029 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 5 min = -2.0 MilliJy,max = 1.9 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 630.36 MicroJy IMAGR3: 2634 Residual map points loaded IMAGR3: Field 5 min Clean flux = 755.433 MicroJy iter= 6446 IMAGR3: Field 5 Clean flux density= 8.716 MilliJy 6446 comps IMAGR3: Total Cleaned flux density = 3.222 Jy 34244 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 1 min = -1.0 MilliJy,max = 988.2 MicroJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 597.38 MicroJy IMAGR3: 3244 Residual map points loaded IMAGR3: Field 1 min Clean flux = -755.837 MicroJy iter= 4800 IMAGR3: Field 1 Clean flux density= 3.139 Jy 4800 comps IMAGR3: Total Cleaned flux density = 3.223 Jy 34329 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 3 min = -1.4 MilliJy,max = 1.6 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 540.30 MicroJy IMAGR3: 6594 Residual map points loaded IMAGR3: Field 3 min Clean flux = 755.485 MicroJy iter= 5505 IMAGR3: Field 3 Clean flux density= 12.847 MilliJy 5505 comps IMAGR3: Total Cleaned flux density = 3.224 Jy 34397 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Field 7 min = -1.5 MilliJy,max = 1.2 MilliJy IMAGR3: BGC Clean: using 103 cell beam + residuals > 413.14 MicroJy IMAGR3: 19977 Residual map points loaded IMAGR3: Field 7 min Clean flux = -749.268 MicroJy iter= 2931 IMAGR3: Field 7 Clean flux density= -17.903 MilliJy 2931 comps IMAGR3: Total Cleaned flux density = 3.224 Jy 34417 comps IMAGR3: VISDFT: Begin DFT component subtraction IMAGR3: I Polarization model processed IMAGR3: Peak residual in window 755.888 less than limit 756.077 MicroJy IMAGR3: Merging the Clean components files IMAGR3: Field 1 compressed from 4800 to 2501 components IMAGR3: Field 2 compressed from 3422 to 1835 components IMAGR3: Field 3 compressed from 5505 to 2729 components IMAGR3: Field 4 compressed from 5575 to 2708 components IMAGR3: Field 5 compressed from 6446 to 3255 components IMAGR3: Field 6 compressed from 5738 to 2879 components IMAGR3: Field 7 compressed from 2931 to 1658 components IMAGR3: Field 1 min = -857.7 MicroJy,max = 931.4 MicroJy IMAGR3: Field 2 min = -1.1 MilliJy,max = 1.3 MilliJy IMAGR3: Field 3 min = -1.4 MilliJy,max = 1.6 MilliJy IMAGR3: Field 4 min = -2.2 MilliJy,max = 1.9 MilliJy IMAGR3: Field 5 min = -2.0 MilliJy,max = 1.8 MilliJy IMAGR3: Field 6 min = -1.7 MilliJy,max = 1.6 MilliJy IMAGR3: Field 7 min = -1.4 MilliJy,max = 1.2 MilliJy IMAGR3: Restoring Clean components IMAGR3: Restoring overlapped Clean components IMAGR3: Restore -8.703 MilliJy ( 105 CCs) from field 1 to field 2 IMAGR3: Restore 19.260 MilliJy ( 381 CCs) from field 1 to field 3 IMAGR3: Restore -7.589 MilliJy ( 432 CCs) from field 1 to field 4 IMAGR3: Restore 9.262 MilliJy ( 377 CCs) from field 1 to field 5 IMAGR3: Restore -17.940 MilliJy ( 507 CCs) from field 1 to field 6 IMAGR3: Restore 22.194 MilliJy ( 172 CCs) from field 1 to field 7 IMAGR3: Restore -3.935 MilliJy ( 82 CCs) from field 2 to field 1 IMAGR3: Restore -13.920 MilliJy ( 141 CCs) from field 2 to field 3 IMAGR3: Restore 10.291 MilliJy ( 197 CCs) from field 2 to field 4 IMAGR3: Restore 3.141 MilliJy ( 114 CCs) from field 3 to field 1 IMAGR3: Restore 4.097 MilliJy ( 93 CCs) from field 3 to field 2 IMAGR3: Restore -12.429 MilliJy ( 192 CCs) from field 3 to field 5 IMAGR3: Restore-660.564 MicroJy ( 154 CCs) from field 4 to field 1 IMAGR3: Restore -5.469 MilliJy ( 84 CCs) from field 4 to field 2 IMAGR3: Restore -3.307 MilliJy ( 165 CCs) from field 4 to field 6 IMAGR3: Restore 551.483 MicroJy ( 209 CCs) from field 5 to field 1 IMAGR3: Restore -3.020 MilliJy ( 271 CCs) from field 5 to field 3 IMAGR3: Restore 76.058 MicroJy ( 106 CCs) from field 5 to field 7 IMAGR3: Restore-170.990 MicroJy ( 126 CCs) from field 6 to field 1 IMAGR3: Restore 12.288 MilliJy ( 203 CCs) from field 6 to field 4 IMAGR3: Restore 2.880 MilliJy ( 99 CCs) from field 6 to field 7 IMAGR3: Restore 2.653 MilliJy ( 45 CCs) from field 7 to field 1 IMAGR3: Restore -2.739 MilliJy ( 164 CCs) from field 7 to field 5 IMAGR3: Restore 7.477 MilliJy ( 102 CCs) from field 7 to field 6 IMAGR3: Checking image max/min IMAGR3: Field 1 final Clean flux 3.141 Jy IMAGR3: Field 2 final Clean flux -5.973 MilliJy IMAGR3: Field 3 final Clean flux 15.166 MilliJy IMAGR3: Field 4 final Clean flux 37.284 MilliJy IMAGR3: Field 5 final Clean flux 2.811 MilliJy IMAGR3: Field 6 final Clean flux 40.907 MilliJy IMAGR3: Field 7 final Clean flux 7.247 MilliJy IMAGR3: Deleting UV work file: IMAGR3: Destroyed 1 extension files of type AN IMAGR3: Destroyed 1 extension files of type FQ IMAGR3: Destroyed UV image file: catno= 9 disk= 1 IMAGR3: Appears to have ended successfully IMAGR3: auto 31DEC06 TST: Cpu= 196.8 Real= 834 TFC@G991216_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 7 disk= 1 AIPS 3: Disk 1 in-CNO 8 renumbered as CNO 6 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.07375 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@0509+101_X,BAND.0-1 >> /home/auto/run/AK485_2000J AIPS 3: AN28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :2 =0509+101' AIPS 3: ' ' AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0509+101_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 8 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 9 disk= 1 AIPS 3: Disk 1 in-CNO 10 renumbered as CNO 7 AIPS 3: Disk 1 in-CNO 11 renumbered as CNO 8 AIPS 3: ' ' AIPS 3: 'ESTIMATED RMS:' '0.126 MILLI JANSKY' AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0137+331_X,BAND.0-1 >& /dev/null AIPS 3: Waiting for returned adverbs AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: cat /tmp/SETFC@0137+331_X,BAND.0-1 >> /home/auto/run/AK485_2000J AIPS 3: AN28_1.log.0 AIPS 3: ' NOW STARTING WITH SOURCE :3 =0137+331' AIPS 3: ' ' AIPS 3: Resumes AIPS 3: SYSTEM command to be executed is: AIPS 3: rm -f /tmp/SETFC@0137+331_X,BAND.0-1 >& /dev/null AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 10 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 11 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 12 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 13 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 14 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 15 disk= 1 AIPS 3: Destroyed 1 extension files of type HI AIPS 3: Destroyed MA image file: catno= 16 disk= 1 AIPS 3: Disk 1 in-CNO 17 renumbered as CNO 9 AIPS 3: Disk 1 in-CNO 18 renumbered as CNO 10 AIPS 3: Disk 1 in-CNO 19 renumbered as CNO 11 AIPS 3: Disk 1 in-CNO 20 renumbered as CNO 12 AIPS 3: Disk 1 in-CNO 21 renumbered as CNO 13 AIPS 3: Disk 1 in-CNO 22 renumbered as CNO 14 AIPS 3: Disk 1 in-CNO 23 renumbered as CNO 15 AIPS 3: ' ' AIPS 3: ' ' AIPS 3: Found in Version=ABIN AIPS 3: '* APPEARS TO HAVE ENDED SUCCESSFULLY *' >>AIPS 3: Disk 1 No files needed renumbering AIPS 3: 'EMPTY CATALOG ?' 15 >AIPS 3: Begin check for any 'standard' scratch files AIPS 3: Scratch files -- destroyed: 0 still active: 0 AIPS 3: User18478: 3432 messages, oldest written 18-SEP-2006 07:41:29 AIPS 3: Deleted 0 messages AIPS 3: Saved POPS environment in area named 'LASTEXIT' AIPS 3: Session command-line history saved. AIPS 3: auto 31DEC06 TST: Cpu= 0.7 Real= 1504 /home/auto/run/AK485_2000JAN28_1.run.0 finished on Mon Sep 18 09:20:12 MDT 2006