Complement to VIII/85A

Source IRAS_F02312+2905: 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 B0231.2+2905                   6.75e+02  1.4e+02      12.00    8520 4   -0.67    4.52  038.5555  +29.3108
 1400  NVSS J023413+291842               2.74e+02  5.5e+01      45.00    8520 4   -0.52    4.00  038.5551  +29.3117
 1400  WB 0231+2905                      3.55e+02  7.1e+01     120.00    8520 4   -0.52    4.00  038.5508  +29.3081
 2380  UGC 2045                          1.75e+02  3.5e+01     162.00    8520 4   -0.68    4.53  038.5558  +29.3106
 4850  87GB 023115.3+290520              1.10e+02  2.2e+01     138.00    8520 4   -0.67    4.52  038.5504  +29.3078
 4850  BWE 0231+2905                     1.09e+02  2.2e+01     138.00    8520 4   -0.68    4.54  038.5508  +29.3081
 4850  GB6 B0231+2905                    1.02e+02  2.0e+01     108.00    8520 4   -0.68    4.53  038.5521  +29.3094
 4850  IRAS F02312+2905                  1.10e+02  2.2e+01     210.00    8520 4   -0.67    4.52  038.5558  +29.3117
 4850  MITG J023415+2918                 8.40e+01  1.7e+01     258.00    8520 4   -0.68    4.54  038.5642  +29.3114

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 J0234.2+2918                 1.07e+03  2.1e+02      79.98    -8520  038.5562  +29.3111
   325  WN B0231.2+2905                   6.75e+02  1.4e+02      12.00     8520  038.5555  +29.3108
  1400  NVSS J023413+291842               2.74e+02  5.5e+01      45.00     8520  038.5551  +29.3117
  1400  WB 0231+2905                      3.55e+02  7.1e+01     120.00     8520  038.5508  +29.3081
  2380  UGC 2045                          1.75e+02  3.5e+01     162.00     8520  038.5558  +29.3106
  4850  87GB 023115.3+290520              1.10e+02  2.2e+01     138.00     8520  038.5504  +29.3078
  4850  MITG J023415+2918                 8.40e+01  1.7e+01     258.00     8520  038.5642  +29.3114

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