Complement to VIII/85A

Source 7C_093721.89+302844.00: 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
151 6C 093723+302901 5.00e+02 1.0e+02 252.00 40168 0 -0.42 3.45 145.0813 +30.2564 151 7C 093721.89+302844.00 3.64e+02 7.3e+01 70.20 40168 0 -0.42 3.45 145.0758 +30.2517 325 WN B0937.3+3028 2.45e+02 4.9e+01 12.00 40168 0 -0.42 3.45 145.0777 +30.2534 1400 FIRST J094018.8+301509 1.10e+02 2.2e+01 5.00 40168 0 -0.43 3.50 145.0785 +30.2528 1400 NVSS J094018+301509 1.40e+02 2.8e+01 45.00 40168 0 -0.43 3.50 145.0787 +30.2526 1400 WB 0937+3028 1.46e+02 2.9e+01 120.00 40168 0 -0.34 3.25 145.0817 +30.2544 4850 87GB 093722.9+302853 1.19e+02 2.4e+01 138.00 40168 0 -0.34 3.25 145.0804 +30.2542 4850 BWE 0937+3028 1.16e+02 2.3e+01 138.00 40168 0 -0.34 3.25 145.0817 +30.2544 4850 GB6 B0937+3028 1.04e+02 2.1e+01 108.00 40168 0 -0.42 3.45 145.0796 +30.2511 4850 MITG J094019+3015 7.80e+01 1.6e+01 258.00 40168 0 -0.42 3.45 145.0808 +30.2564 8400 CLASS J094018.8460+301509.948 5.62e+01 1.1e+01 0.33 40168 0 -0.34 3.25 145.0785 +30.2528 15000 9C J0940+3015 6.60e+01 1.3e+01 25.20 40168 0 -0.38 3.36 145.0783 +30.2525

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
151 6C 093723+302901 5.00e+02 1.0e+02 252.00 40168 145.0813 +30.2564 151 7C 093721.89+302844.00 3.64e+02 7.3e+01 70.20 40168 145.0758 +30.2517 325 WN B0937.3+3028 2.45e+02 4.9e+01 12.00 40168 145.0777 +30.2534 365 TXS 0937+304 2.00e+02 4.0e+01 6.00 -40168 145.0627 +30.2668 408 B2.1 0937+30 2.20e+02 4.4e+01 0.00 -40168 145.0771 +30.2600 1400 FIRST J094017.1+301504 7.20e+00 1.4e+00 5.00 -40168 145.0717 +30.2512 1400 FIRST J094017.9+301506 7.30e+00 1.5e+00 5.00 -40168 145.0748 +30.2518 1400 FIRST J094018.8+301509 1.10e+02 2.2e+01 5.00 40168 145.0785 +30.2528 1400 FIRST J094019.6+301510 1.97e+01 3.9e+00 5.00 -40168 145.0820 +30.2530 1400 NVSS J094018+301509 1.40e+02 2.8e+01 45.00 40168 145.0787 +30.2526 1400 WB 0937+3028 1.46e+02 2.9e+01 120.00 40168 145.0817 +30.2544 4850 GB6 B0937+3028 1.04e+02 2.1e+01 108.00 40168 145.0796 +30.2511 4850 MITG J094019+3015 7.80e+01 1.6e+01 258.00 40168 145.0808 +30.2564 8400 CLASS J094018.8460+301509.948 5.62e+01 1.1e+01 0.33 40168 145.0785 +30.2528 15000 9C J0940+3015 6.60e+01 1.3e+01 25.20 40168 145.0783 +30.2525

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