Complement to VIII/85A

Source VLSS_J0939.3+4016: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
Adapt
Plot
nu
S
x cuts: xlog Bitmap size:
y cuts: ylog
"-c="

The 2 columns in color are computed by VizieR, and are not part of the original data.
The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/spectra
Post annotation
SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
The parameters of the radio spectra[image][spectrum] (631736 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq n a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
74 VLSS J0939.3+4016 9.81e+03 2.0e+03 79.98 40132 4 -1.02 5.97 144.8350 +40.2800 151 6C 093613+403028 5.70e+03 1.1e+03 252.00 40132 4 -1.09 6.18 144.8338 +40.2814 151 7C 093613.50+403026.00 5.59e+03 1.1e+03 70.20 40132 4 -1.04 6.03 144.8346 +40.2808 178 4C +40.23 3.80e+03 1.1e+03 690.00 40132 4 -1.03 6.00 144.8321 +40.2833 232 MY 093613.6+401648.8 4.12e+03 8.2e+02 150.00 40132 4 -1.02 5.99 144.8350 +40.2802 325 WN B0936.2+4030 2.77e+03 5.5e+02 12.00 40132 4 -1.02 5.97 144.8347 +40.2804 365 TXS 0936+405 2.74e+03 5.5e+02 6.00 40132 4 -1.08 6.15 144.8348 +40.2807 408 B3 0936+405 2.12e+03 4.2e+02 84.00 40132 4 -1.02 5.97 144.8350 +40.2806 1400 NVSS J093920+401650 6.03e+02 1.2e+02 45.00 40132 4 -1.04 6.03 144.8350 +40.2807 1400 WB 0936+4030 5.59e+02 1.1e+02 120.00 40132 4 -1.09 6.18 144.8254 +40.2822 4730 B3a 0936+405 1.43e+02 2.9e+01 168.00 40132 4 -1.10 6.20 144.8351 +40.2805 4850 87GB 093611.2+403031 1.64e+02 3.3e+01 138.00 40132 4 -1.04 6.03 144.8250 +40.2822 4850 BWE 0936+4030 1.44e+02 2.9e+01 138.00 40132 4 -1.09 6.18 144.8254 +40.2822 4850 GB6 B0936+4030 1.42e+02 2.8e+01 108.00 40132 4 -1.04 6.03 144.8313 +40.2811

The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/waste
Post annotation
SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
Source parameters based on positional cross-id[spectrum] (1497216 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
74 VLSS J0939.3+4016 9.81e+03 2.0e+03 79.98 40132 144.8350 +40.2800 151 6C 093613+403028 5.70e+03 1.1e+03 252.00 40132 144.8338 +40.2814 178 4C +40.23 3.80e+03 1.1e+03 690.00 40132 144.8321 +40.2833 232 MY 093613.6+401648.8 4.12e+03 8.2e+02 150.00 40132 144.8350 +40.2802 325 WN B0936.0+4036 1.50e+01 4.0e+00 12.00 -40132 144.7848 +40.3745 325 WN B0936.2+4030 2.77e+03 5.5e+02 12.00 40132 144.8347 +40.2804 408 B3 0936+405 2.12e+03 4.2e+02 84.00 40132 144.8350 +40.2806 1400 FIRST J093920.0+401638 3.14e+02 6.3e+01 5.00 -40132 144.8335 +40.2772 1400 FIRST J093920.7+401705 2.66e+02 5.3e+01 5.00 -40132 144.8364 +40.2849 1400 NVSS J093909+402217 6.90e+00 1.4e+00 45.00 -40132 144.7885 +40.3714 1400 NVSS J093920+401650 6.03e+02 1.2e+02 45.00 40132 144.8350 +40.2807 4730 B3a 0936+405 1.43e+02 2.9e+01 168.00 40132 144.8351 +40.2805 4850 87GB 093611.2+403031 1.64e+02 3.3e+01 138.00 40132 144.8250 +40.2822 10600 B3VLA 518 4.16e+01 8.3e+00 69.00 -40132 144.8354 +40.2808

Note: For the spectrum finding algorithm, the errors have been increased by 50%