Complement to VIII/85A

Source GB6_B0651+4251: 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 7C 065109.30+425147.00 3.89e+02 7.8e+01 70.20 25473 1 -0.18 2.93 103.6804 +42.7994 325 WN B0651.1+4251 3.02e+02 6.0e+01 12.00 25473 1 -0.18 2.92 103.6831 +42.7999 325 WN B0651.1+4251A 2.81e+02 5.6e+01 12.00 25473 1 -0.20 2.97 103.6816 +42.7997 408 B3 0651+428 2.80e+02 5.6e+01 84.00 25473 1 -0.20 2.97 103.6771 +42.8006 1400 NVSS J065443+424759 2.02e+02 4.0e+01 45.00 25473 1 -0.20 2.97 103.6816 +42.7997 1400 WB 0651+4251 1.88e+02 3.8e+01 120.00 25473 1 -0.18 2.92 103.6821 +42.8008 2700 RGB11 J0654.7+4247 2.66e+02 5.3e+01 258.00 25473 1 -0.18 2.92 103.6817 +42.8000 4850 87GB 065109.5+425150 2.09e+02 4.2e+01 138.00 25473 1 -0.18 2.92 103.6813 +42.8003 4850 BWE 0651+4251 1.85e+02 3.7e+01 138.00 25473 1 -0.18 2.93 103.6821 +42.8008 4850 GB6 B0651+4251 1.90e+02 3.8e+01 108.00 25473 1 -0.18 2.92 103.6813 +42.8000 4885 RGB 0654+427 1.90e+02 3.8e+01 4.02 25473 1 -0.18 2.92 103.6814 +42.7996 5000 RGB6 J0654.7+4247 1.77e+02 3.5e+01 144.00 25473 1 -0.18 2.92 103.6817 +42.8000 8400 CLASS J065443.5268+424758.719 1.50e+02 3.0e+01 0.33 25473 1 -0.18 2.92 103.6813 +42.7996 8400 JVAS J0654+427 1.49e+02 3.0e+01 0.33 25473 1 -0.20 2.97 103.6814 +42.7996 10700 RGB2 J0654.7+4247 1.43e+02 2.9e+01 72.00 25473 1 -0.18 2.92 103.6817 +42.8000

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 7C 065109.30+425147.00 3.89e+02 7.8e+01 70.20 25473 103.6804 +42.7994 232 MY 065110.2+424820.3 6.70e+02 1.3e+02 150.00 -25473 103.6842 +42.8056 325 WN B0651.1+4251A 2.81e+02 5.6e+01 12.00 25473 103.6816 +42.7997 325 WN B0651.1+4251B 1.90e+01 3.9e+00 12.00 -25473 103.7114 +42.7814 408 B3 0651+428 2.80e+02 5.6e+01 84.00 25473 103.6771 +42.8006 1400 NVSS J065453+424703 4.00e+00 8.0e-01 45.00 -25473 103.7212 +42.7842 1400 WB 0651+4251 1.88e+02 3.8e+01 120.00 25473 103.6821 +42.8008 4850 87GB 065109.5+425150 2.09e+02 4.2e+01 138.00 25473 103.6813 +42.8003 4850 GB6 B0651+4251 1.90e+02 3.8e+01 108.00 25473 103.6813 +42.8000 4885 RGB 0654+427 1.90e+02 3.8e+01 4.02 25473 103.6814 +42.7996 5000 RGB6 J0654.7+4247 1.77e+02 3.5e+01 144.00 25473 103.6817 +42.8000 8400 CLASS J065443.5268+424758.719 1.50e+02 3.0e+01 0.33 25473 103.6813 +42.7996

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