Complement to VIII/85A

Source CLASS_J162028.2097+032453.323: 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]
2010A&A...511A..53V

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  


  365  TXS 1617+035                      3.75e+02  7.5e+01       6.00   68269 0   -0.63    4.19  245.1176  +03.4150
 1400  FIRST J162028.2+032453            1.47e+02  2.9e+01       5.00   68269 0   -0.63    4.19  245.1176  +03.4148
 1400  NVSS J162028+032453               1.50e+02  3.0e+01      45.00   68269 0   -0.63    4.19  245.1173  +03.4147
 4850  87GB 161757.5+033206              1.29e+02  2.6e+01     138.00   68269 0   -0.68    4.46  245.1150  +03.4164
 4850  BWE 1617+0332                     1.25e+02  2.5e+01     138.00   68269 0   -0.68    4.46  245.1150  +03.4175
 4850  GB6 B1617+0331                    1.29e+02  2.6e+01     108.00   68269 0   -0.68    4.46  245.1158  +03.4131
 4850  MITG J162027+0325                 9.90e+01  2.0e+01     258.00   68269 0   -0.68    4.46  245.1163  +03.4181
 4850  PMN J1620+0325                    7.30e+01  1.5e+01     168.00   68269 0   -0.68    4.46  245.1275  +03.4222
 8400  CLASS J162028.2097+032453.323     6.11e+01  1.2e+01       0.33   68269 0   -0.63    4.19  245.1175  +03.4148

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]
2010A&A...511A..53V

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 J1620.4+0324                 1.53e+03  3.1e+02      79.98   -68269  245.1183  +03.4149
   365  TXS 1617+035                      3.75e+02  7.5e+01       6.00    68269  245.1176  +03.4150
  1400  NVSS J162028+032453               1.50e+02  3.0e+01      45.00    68269  245.1173  +03.4147
  4850  87GB 161757.5+033206              1.29e+02  2.6e+01     138.00    68269  245.1150  +03.4164
  4850  GB6 B1617+0331                    1.29e+02  2.6e+01     108.00    68269  245.1158  +03.4131
  4850  PMN J1620+0325                    7.30e+01  1.5e+01     168.00    68269  245.1275  +03.4222
  8400  CLASS J162028.2097+032453.323     6.11e+01  1.2e+01       0.33    68269  245.1175  +03.4148

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