Complement to VIII/85A

Source GB6_B0838+4536: 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 083849.60+453626.00            1.17e+02  2.9e+01      70.20   33820 0   -0.17    2.41  130.5637  +45.4278
  325  WN B0838.8+4536                   7.80e+01  1.6e+01      12.00   33820 0   -0.16    2.38  130.5644  +45.4283
  327  WSTB 64W176                       8.06e+01  1.6e+01      90.00   33820 0   -0.11    2.17  130.5655  +45.4273
  327  WSTBa 64W2290                     9.52e+01  1.9e+01      60.00   33820 0   -0.17    2.41  130.5650  +45.4282
 1400  FIRST J084215.3+452544            6.77e+01  1.4e+01       5.00   33820 0   -0.13    2.25  130.5639  +45.4289
 1400  NVSS J084215+452543               7.40e+01  1.5e+01      45.00   33820 0   -0.17    2.41  130.5643  +45.4286
 1412  WSTB 55W106                       7.56e+01  1.5e+01      23.10   33820 0   -0.17    2.40  130.5644  +45.4291
 4850  87GB 083849.4+453638              5.88e+01  1.2e+01     138.00   33820 0   -0.18    2.43  130.5629  +45.4311
 4850  BWE 0838+4536                     4.90e+01  9.8e+00     138.00   33820 0   -0.17    2.41  130.5671  +45.4308
 4850  GB6 B0838+4536                    6.05e+01  1.2e+01     108.00   33820 0   -0.17    2.41  130.5629  +45.4297
 8400  CLASS J084215.3527+452544.182     5.32e+01  1.1e+01       0.33   33820 0   -0.18    2.43  130.5640  +45.4289

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 083849.60+453626.00            1.17e+02  2.9e+01      70.20    33820  130.5637  +45.4278
   327  WSTB 64W176                       8.06e+01  1.6e+01      90.00    33820  130.5655  +45.4273
   327  WSTBa 64W2290                     9.52e+01  1.9e+01      60.00    33820  130.5650  +45.4282
  1400  FIRST J084216.2+452516            4.00e+00  8.0e-01       5.00   -33820  130.5677  +45.4214
  4850  GB6 B0838+4536                    6.05e+01  1.2e+01     108.00    33820  130.5629  +45.4297

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