Complement to VIII/85A

Source 6C_065111+541250: 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 J0655.1+5410                 2.67e+03  5.8e+02      79.98  -146978  103.7900  +54.1817
   151  6C 065111+541250                  2.08e+04  4.2e+03     252.00  -146978  103.8117  +54.1497
   178  3CR 171                           2.30e+04  4.6e+03     360.00  -146978  103.8275  +54.1417
  1400  FIRST J065509.8+541048            2.20e+00  4.0e-01       5.00  -146978  103.7909  +54.1801
  4850  GB6 B0651+5412                    1.15e+03  2.3e+02     108.00  -146978  103.8046  +54.1525

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