Complement to VIII/85A

Source CLASS_J073552.7434+203638.831: 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 0732+207                      2.23e+02  4.5e+01       6.00   31454 0   -0.16    2.74  113.9695  +20.6114
 1400  FIRST J073552.7+203638            1.75e+02  3.5e+01       5.00   31454 0   -0.17    2.78  113.9697  +20.6108
 1400  NVSS J073552+203639               1.50e+02  3.0e+01      45.00   31454 0   -0.17    2.78  113.9698  +20.6108
 1400  WB 0732+2043                      1.33e+02  2.7e+01     120.00   31454 0   -0.17    2.78  113.9688  +20.6178
 4850  87GB 073255.6+204345              1.64e+02  3.3e+01     138.00   31454 0   -0.16    2.74  113.9683  +20.6178
 4850  BWE 0732+2043                     1.60e+02  3.2e+01     138.00   31454 0   -0.13    2.68  113.9688  +20.6178
 4850  GB6 B0732+2043                    1.44e+02  2.9e+01     108.00   31454 0   -0.16    2.74  113.9688  +20.6158
 4850  MITG J073552+2035                 1.08e+02  2.2e+01     258.00   31454 0   -0.13    2.60  113.9671  +20.5925
 8400  CLASS J073552.7434+203638.831     1.54e+02  3.1e+01       0.33   31454 0   -0.16    2.74  113.9697  +20.6108
 8400  JVAS J0735+2036                   1.54e+02  3.1e+01       0.33   31454 0   -0.16    2.74  113.9698  +20.6108

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  


   365  TXS 0732+207                      2.23e+02  4.5e+01       6.00    31454  113.9695  +20.6114
  1400  WB 0732+2043                      1.33e+02  2.7e+01     120.00    31454  113.9688  +20.6178
  4850  BWE 0732+2043                     1.60e+02  3.2e+01     138.00    31454  113.9688  +20.6178
  4850  GB6 B0732+2043                    1.44e+02  2.9e+01     108.00    31454  113.9688  +20.6158
  4850  MITG J073552+2035                 1.08e+02  2.2e+01     258.00    31454  113.9671  +20.5925
  8400  CLASS J073552.7434+203638.831     1.54e+02  3.1e+01       0.33    31454  113.9697  +20.6108

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