VLA calibrator information for 0149+0555

This page summarizes the information for 0149+0555 as found in the original VLA calibrator list and, if found there, a link to search the NRAO VLA Archive Survey (NVAS) for calibrator data before 2010. Furthermore, a table with the most recent approximate flux densities, starting from 2017 as mined from the VLA CASA pipeline is presented.

If shown at the top, we have recovered the original, pre-WIDAR ANTSOL flux density solutions from the period roughly 2000-2007; symbols as explained next.
The mined data are plotted (gray, on the left hand side) as function of (log) frequency on the top and as function of time on the bottom. The frequency band symbols in the bottom panel follow the symbols as outlined in the top panel:

4-band  (~75 MHz) horizontal stripe       X-band (~10.0 GHz) cross
P-band (~350 MHz) open triangle        U/Ku-band (~15.0 GHz) filled square
L-band (~1.5 GHz) VLA-Y shape             K-band (~22.2 GHz) open circle
S-band (~3.0 GHz) filled triangle      A/Ka-band (~33.2 GHz) 6-pointed star
C-band (~6.0 GHz) open square             Q-band (~45.0 GHz) filled circle
Assume a 10% flux density error on each point, up to 30% for the higher frequency data points. The dashed lines in the frequency plot indicate the approximate spectral index in the frequency band (tied to the measured flux density).
Depending on the spectral behavior, different receiver observing bands (as indicated with the log-frequency axis) may have very different typical flux densities. Note that there can be significant flux density changes for different array configurations, which start date is indicated at the top of the time-line figure. Calendar years are separated by vertical dotted lines.
If shown, a curve depicts a fit to the (unweighted) average data for each band (if there are more than two bands with measured flux densities). The fit equation is listed at the top where the x-coordinate represents the base-10 log of the frequency (GHz) and the y-coordinate represents the base-10 log of the flux density (mJy/bm). The fit may use more data than shown and is using data with different time stamps, which means typically different flux densitities in a single band for genuine variable sources (and/or observed in different array configurations).
Depending on the variability of the source, array configuration and the quality of the data, this fit may, or may not, be representative for the data!

(Click on the figure for a larger view in a new tab/window)

 Original (outdated) VLA calibrator list information: 
 IAU NAME EQUINOX  PC RA(hh,mm,ss)    DEC(ddd,mm,ss)   POS.REF ALT.NAME
 ===================================================================
 0149+059   J2000  A 01h49m22.370886s  05d55'53.568660"  Aug01         
 0146+056   B1950  A 01h46m45.525100s  05d41'00.797000"
 -----------------------------------------------------
 BAND        A B C D    FLUX(Jy)    UVMIN(kL)  UVMAX(kL)
 =====================================================
  20cm    L  S S S S       0.60
   6cm    C  P P P P       0.89
 3.7cm    X  P P P P       1.16
   2cm    U  S S S S       0.75
 0.7cm    Q  W W W W       0.6

Default NVAS search around this position (in new tab/window)

WARNING: multiple positions found, using first one 027.3432083 +05.9315278 027.3432120 +05.9315469 Results from CASA pipeline flux density mining:
Observing date (UT)Flux density (Jy/bm)Source name used
S-band data (filled triangles)
201707071.038CL8-0149+059
201705201.082J0149+0555
201706171.0440149+059
201707291.063J0149+0555
201710131.072J0149+0555
201711031.089J0149+0555
201711151.141J0149+0555
201712011.047J0149+0555
201712051.059J0149+0555
201712091.099J0149+0555
201712141.075J0149+0555
201712141.091J0149+0555
201712151.088J0149+0555
201712181.074J0149+0555
201712191.050J0149+0555
201712192.923J0149+0555
201804221.031J0149+0555
201804221.093J0149+0555
201804221.087J0149+0555
201804261.084J0149+0555
201907290.999J0149+0555
201910101.028J0149+0555
201910161.013J0149+0555
201607291.050J0149+0555
201705281.082J0149+0555
201706173.0980149+059
201709041.074J0149+0555
201709051.074J0149+0555
201709271.038J0149+0555
201709271.040J0149+0555
201710201.052J0149+0555
201710251.057J0149+0555
201712151.061J0149+0555
201712151.070J0149+0555
201910100.976J0149+0555
202009260.955J0149+0555
C-band data (open squares)
201706010.966J0149+0555
201706140.961J0149+0555
201706160.963J0149+0555
201706170.974J0149+0555
201706171.171J0149+0555
201706170.940J0149+0555
201706170.957J0149+0555
201706180.969J0149+0555
201706251.036J0149+0555
201706300.963J0149+0555
201706300.958J0149+0555
201707020.972J0149+0555
201707060.961J0149+0555
201707070.980J0149+0555
201707101.196J0149+0555
201707110.960J0149+0555
201707110.955J0149+0555
201707131.436J0149+0555
201707260.970J0149+0555
201708020.957J0149+0555
201708030.963J0149+0555
201708060.975J0149+0555
201708090.967J0149+0555
201708220.957J0149+0555
201708280.971J0149+0555
201708300.961J0149+0555
201708300.961J0149+0555
201708300.960J0149+0555
201708310.955J0149+0555
201708310.955J0149+0555
201708310.953J0149+0555
201709120.945J0149+0555
201709230.958J0149+0555
201709230.949J0149+0555
201709250.955J0149+0555
201709260.957J0149+0555
201709280.945J0149+0555
201710020.945J0149+0555
201710060.939J0149+0555
201710270.933J0149+0555
201710310.950J0149+0555
201710310.949J0149+0555
201711010.935J0149+0555
201711020.934J0149+0555
201711020.934J0149+0555
201711040.940J0149+0555
201711050.942J0149+0555
201711050.937J0149+0555
201711060.930J0149+0555
201711060.939J0149+0555
201711080.937J0149+0555
201711090.945J0149+0555
201711130.926J0149+0555
201711140.928J0149+0555
201711160.944J0149+0555
201711220.940J0149+0555
201712040.935J0149+0555
201712060.949J0149+0555
201712060.945J0149+0555
201712070.934J0149+0555
201712070.935J0149+0555
201804080.882J0149+0555
201812070.988J0149+0555
201901290.958J0149+0555
201903190.955J0149+0555
X-band data (X-crosses)
201802220.818J0149+0555
201802220.820J0149+0555
201804050.820J0149+0555
201908200.713J0149+0555
202104240.723J0149+0555
K-band data (open circles)
201706140.646J0149+0555
201708220.643J0149+0555