Complement to VIII/85A

Source GB6_B0423+2945: 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  


  325  WN B0423.3+2945                   2.68e+02  5.4e+01      12.00   16983 0   -0.16    2.90  066.6262  +29.8736
  365  TXS 0423+297                      3.20e+02  6.4e+01       6.00   16983 0   -0.16    2.90  066.6266  +29.8732
 1400  NVSS J042630+295223               2.53e+02  5.1e+01      45.00   16983 0   -0.16    2.90  066.6261  +29.8731
 4850  87GB 042322.0+294543              2.02e+02  4.0e+01     138.00   16983 0   -0.16    2.90  066.6283  +29.8742
 4850  BWE 0423+2945                     2.02e+02  4.0e+01     138.00   16983 0   -0.16    2.90  066.6287  +29.8742
 4850  GB6 B0423+2945                    2.26e+02  4.5e+01     108.00   16983 0   -0.16    2.90  066.6258  +29.8731
 4850  MITG J042629+2952                 2.24e+02  4.5e+01     258.00   16983 0   -0.16    2.90  066.6225  +29.8786
 4850  MITG J042630+2952                 2.22e+02  4.4e+01     258.00   16983 0   -0.16    2.90  066.6262  +29.8781
 8400  CLASS J042630.2281+295222.899     1.91e+02  3.8e+01       0.33   16983 0   -0.16    2.90  066.6259  +29.8730
 8400  JVAS J0426+2952                   1.88e+02  3.8e+01       0.33   16983 0   -0.17    2.93  066.6260  +29.8730

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  


   325  WN B0423.3+2945                   2.68e+02  5.4e+01      12.00    16983  066.6262  +29.8736
   365  TXS 0423+297                      3.20e+02  6.4e+01       6.00    16983  066.6266  +29.8732
  1400  WB 0423+2945                      1.67e+02  3.3e+01     120.00   -16983  066.6287  +29.8742
  4850  BWE 0423+2945                     2.02e+02  4.0e+01     138.00    16983  066.6287  +29.8742
  4850  GB6 B0423+2945                    2.26e+02  4.5e+01     108.00    16983  066.6258  +29.8731
  8400  CLASS J042630.2281+295222.899     1.91e+02  3.8e+01       0.33    16983  066.6259  +29.8730

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