Complement to VIII/85A

Source NVSS_J051342-201611: 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  


   74  VLSS J0513.7-2016                 1.00e+03  2.0e+02      79.98   21011 0   -0.57    4.06  078.4292  -20.2707
  325  WISH B0511.5-2019                 3.82e+02  7.6e+01      18.00   21011 0   -0.57    4.06  078.4287  -20.2690
  365  TXS 0511-203                      4.03e+02  8.1e+01       6.00   21011 0   -0.57    4.06  078.4289  -20.2695
 1400  NVSS J051342-201611               1.97e+02  3.9e+01      45.00   21011 0   -0.57    4.06  078.4286  -20.2698
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
No object found

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