Complement to VIII/85A

Source JVAS_J0833+1123: 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 +11.28                         5.00e+03  1.5e+03     690.00  -154049  128.3350  +11.4817
  1400  FIRST J083314.3+112336            4.26e+02  8.5e+01       5.00  -154049  128.3099  +11.3934
  4850  87GB 083029.8+113412              3.36e+02  6.7e+01     138.00  -154049  128.3092  +11.3989
  4850  MITG J083315+1123                 2.40e+02  4.8e+01     258.00  -154049  128.3137  +11.3942
  8400  JVAS J0833+1123                   3.43e+02  6.9e+01       0.33  -154049  128.3099  +11.3934

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