VLA calibrator information for 0555+3948

This page summarizes the information for 0555+3948 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
 ===================================================================
 0555+398   J2000  A 05h55m30.805608s  39d48'49.165000"  Aug01         
 0552+398   B1950  A 05h52m01.407200s  39d48'21.946000"
 -----------------------------------------------------
 BAND        A B C D    FLUX(Jy)    UVMIN(kL)  UVMAX(kL)
 =====================================================
  20cm    L  P P P P       1.70
   6cm    C  P P P P       5.00
 3.7cm    X  P P P P       6.20
   2cm    U  P P P P       2.80
 0.7cm    Q  S S S S       2.5

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

Results from CASA pipeline flux density mining:
Observing date (UT)Flux density (Jy/bm)Source name used
L-band data ("VLA Y-arm" symbols)
201712102.011J0555+3948
201907291.770J0555+3948
201910161.781J0555+3948
202305291.817J0555+3948
S-band data (filled triangles)
201709093.913J0555+3948
201712104.138J0555+3948
201811291.582J0555+3948
201905033.835J0555+3948
202112093.858J0555+3948
C-band data (open squares)
201705274.140J0555+3948
201708124.038J0555+3948
201710314.227J0555+3948
201711254.045J0555+3948
201712104.146J0555+3948
201811182.162J0555+3948
201904063.822J0555+3948
201908043.848J0555+3948
X-band data (X-crosses)
201712103.201J0555+3948
201802103.149J0555+3948
U-band data (filled squares)
201706082.131J0555+3948
201706102.311J0555+3948
201706112.257J0555+3948
201708102.251J0555+3948
K-band data (open circles)
201705291.792J0555+3948
201706031.796J0555+3948
201706161.829J0555+3948
201708101.831J0555+3948
201712101.991J0555+3948
201811222.365J0555+3948