Complement to VIII/85A

Source B2.1_1656+29: 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 B1656.0+2921                   2.22e+02  4.4e+01      12.00   73230 0   -0.78    4.40  254.5077  +29.2868
  408  B2.1 1656+29                      2.50e+02  5.0e+01       0.00   73230 0   -0.78    4.40  254.5021  +29.2667
  408  B2.2 1656+29                      2.47e+02  4.9e+01       0.00   73230 0   -0.80    4.48  254.5146  +29.2933
 4850  BWE 1656+2921                     3.60e+01  7.2e+00     138.00   73230 0   -0.80    4.48  254.5096  +29.2875
 4850  GB6 B1656+2921                    3.24e+01  6.5e+00     108.00   73230 0   -0.80    4.48  254.5083  +29.2853
 4885  RGB 1658+292                      2.70e+01  5.4e+00       4.02   73230 0   -0.80    4.48  254.5039  +29.2869

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 J1658.0+2917                 8.50e+02  1.7e+02      79.98   -73230  254.5075  +29.2869
   151  7C 165604.09+292142.00            5.28e+02  1.1e+02      70.20   -73230  254.5071  +29.2861
   325  WN B1656.0+2921                   2.22e+02  4.4e+01      12.00    73230  254.5077  +29.2868
   408  B2.1 1656+29                      2.50e+02  5.0e+01       0.00    73230  254.5021  +29.2667
  1400  FIRST J165801.0+291712            3.64e+01  7.3e+00       5.00   -73230  254.5044  +29.2867
  1400  FIRST J165802.4+291702            4.40e+01  8.8e+00       5.00   -73230  254.5101  +29.2842
  1400  NVSS J165801+291707               8.04e+01  1.6e+01      45.00   -73230  254.5076  +29.2853
  4850  87GB 165604.4+292143              5.47e+01  1.1e+01     138.00   -73230  254.5087  +29.2864
  4850  BWE 1656+2921                     3.60e+01  7.2e+00     138.00    73230  254.5096  +29.2875
  4850  GB6 B1656+2921                    3.24e+01  6.5e+00     108.00    73230  254.5083  +29.2853
  4885  RGB 1658+292                      2.70e+01  5.4e+00       4.02    73230  254.5039  +29.2869

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