Complement to VIII/85A

Source WB_0950+7925: 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
38 8C 095018+792551 5.30e+03 1.1e+03 270.00 103944 4 -0.68 4.80 148.9917 +79.1942 74 VLSS J0955.9+7911 3.17e+03 6.3e+02 79.98 103944 4 -0.68 4.80 148.9996 +79.1936 151 6C 095020+792546 2.34e+03 4.7e+02 252.00 103944 4 -0.68 4.80 148.9996 +79.1928 151 7C 095019.89+792551.00 2.35e+03 4.7e+02 70.20 103944 4 -0.68 4.80 148.9988 +79.1939 232 MY 095019.0+791137.3 1.55e+03 3.1e+02 150.00 103944 4 -0.68 4.80 148.9950 +79.1937 325 WN B0950.3+7925 1.30e+03 2.6e+02 12.00 103944 4 -0.68 4.80 148.9982 +79.1929 1400 NVSS J095559+791134 4.15e+02 8.3e+01 45.00 103944 4 -0.68 4.80 148.9992 +79.1930 1400 WB 0950+7925 3.71e+02 7.4e+01 120.00 103944 4 -0.68 4.80 148.9575 +79.1825
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
No object found

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