Complement to VIII/85A

Source GB6_B1037+0633: 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  


   178  4C +06.41                         2.80e+03  8.4e+02     690.00  -178878  160.1942  +06.3300
  4850  87GB 103758.5+063247              9.85e+01  2.0e+01     138.00  -178878  160.1450  +06.2853
  4850  BWE 1037+0633                     5.50e+01  1.1e+01     138.00  -178878  160.1421  +06.2886
  4850  GB6 B1037+0633                    7.15e+01  1.4e+01     108.00  -178878  160.1342  +06.2900
  8400  CLASS J104034.6595+061650.216     2.00e+00  4.0e-01       0.33  -178878  160.1444  +06.2806

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