Complement to VIII/85A

Source GB6_B2127+0831: 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  


 1400  WB 2127+0830                      3.20e+02  6.4e+01     120.00   88102 0   -0.46    3.96  322.5733  +08.7358
 4850  87GB 212749.9+083056              1.82e+02  3.6e+01     138.00   88102 0   -0.45    3.93  322.5729  +08.7356
 4850  GB6 B2127+0831                    1.80e+02  3.6e+01     108.00   88102 0   -0.45    3.93  322.5713  +08.7367
 8400  CLASS J213016.2529+084355.908     1.35e+02  2.7e+01       0.33   88102 0   -0.48    4.03  322.5677  +08.7322
 8400  JVAS J2130+0843                   1.42e+02  2.8e+01       0.33   88102 0   -0.45    3.93  322.5677  +08.7322

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  


  1400  NVSS J213012+084540               2.30e+00  5.0e-01      45.00   -88102  322.5540  +08.7612
  1400  NVSS J213016+084356               1.43e+02  2.8e+01      45.00   -88102  322.5678  +08.7322
  1400  WB 2127+0830                      3.20e+02  6.4e+01     120.00    88102  322.5733  +08.7358
  4850  87GB 212749.9+083056              1.82e+02  3.6e+01     138.00    88102  322.5729  +08.7356
  4850  BWE 2127+0830                     1.83e+02  3.7e+01     138.00   -88102  322.5733  +08.7358
  4850  GB6 B2127+0831                    1.80e+02  3.6e+01     108.00    88102  322.5713  +08.7367
  4850  MITG J213016+0843                 3.51e+02  7.0e+01     258.00   -88102  322.5692  +08.7286
  4850  PMN J2130+0843                    3.35e+02  6.7e+01     168.00   -88102  322.5638  +08.7328
  8400  CLASS J213016.1842+084352.856     1.90e+00  4.0e-01       0.33   -88102  322.5674  +08.7313
  8400  CLASS J213016.1980+084352.570     3.40e+00  7.0e-01       0.33   -88102  322.5674  +08.7313
  8400  CLASS J213016.2529+084355.908     1.35e+02  2.7e+01       0.33    88102  322.5677  +08.7322
  8400  CLASS J213016.5549+084348.021     2.80e+00  6.0e-01       0.33   -88102  322.5690  +08.7300

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