Complement to VIII/85A

Source MRC_0736-062: 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="

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
No object foundThe 1 column 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/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 J0739.1-0623                 1.23e+03  2.5e+02      79.98  -164294  114.7842  -06.3841
   408  MRC 0736-062                      9.00e+02  1.8e+02     120.00  -164294  114.7854  -06.3783
  1400  NVSS J073906-062331               4.00e+00  8.0e-01      45.00  -164294  114.7785  -06.3921
  1400  NVSS J073908-062243               2.87e+02  5.7e+01      45.00  -164294  114.7862  -06.3786
  4850  PMN J0738-0626                    1.10e+03  2.2e+02     168.00  -164294  114.7408  -06.4478

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