Complement to VIII/85A

Source CLASS_J150509.0111+331832.517: 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  


  151  7C 150307.09+333003.00            1.59e+02  3.4e+01      70.20   65825 0   -0.16    2.56  226.2879  +33.3075
  325  WN B1503.1+3330                   1.67e+02  3.3e+01      12.00   65825 0   -0.16    2.56  226.2877  +33.3088
 1400  FIRST J150508.9+331832            1.01e+02  2.0e+01       5.00   65825 0   -0.20    2.64  226.2875  +33.3091
 1400  NVSS J150508+331832               1.11e+02  2.2e+01      45.00   65825 0   -0.16    2.55  226.2873  +33.3090
 4850  87GB 150308.1+332959              7.90e+01  1.6e+01     138.00   65825 0   -0.16    2.56  226.2925  +33.3067
 4850  BWE 1503+3330                     7.60e+01  1.5e+01     138.00   65825 0   -0.16    2.55  226.2929  +33.3069
 4850  GB6 B1503+3330                    7.70e+01  1.5e+01     108.00   65825 0   -0.16    2.56  226.2929  +33.3086
 4850  MITG J150512+3318                 6.20e+01  1.2e+01     258.00   65825 0   -0.34    3.06  226.3033  +33.3119
 8400  CLASS J150509.0111+331832.517     1.15e+02  2.3e+01       0.33   65825 0   -0.16    2.56  226.2876  +33.3090

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  


   151  7C 150307.09+333003.00            1.59e+02  3.4e+01      70.20    65825  226.2879  +33.3075
   325  WN B1503.1+3330                   1.67e+02  3.3e+01      12.00    65825  226.2877  +33.3088
   408  B2.1 1503+33                      2.50e+02  5.0e+01       0.00   -65825  226.2883  +33.2983
  1400  FIRST J150508.9+331832            1.01e+02  2.0e+01       5.00    65825  226.2875  +33.3091
  1400  NVSS J150508+331832               1.11e+02  2.2e+01      45.00    65825  226.2873  +33.3090
  4850  MITG J150512+3318                 6.20e+01  1.2e+01     258.00    65825  226.3033  +33.3119
  8400  CLASS J150509.0111+331832.517     1.15e+02  2.3e+01       0.33    65825  226.2876  +33.3090

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