Complement to VIII/85A

Source WB_1435+2834: 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  


   74  VLSS J1438.1+2821                 6.30e+03  1.3e+03      79.98   60148 0   -0.78    5.31  219.5425  +28.3628
  178  4C +28.36                         3.60e+03  1.1e+03     690.00   60148 0   -0.83    5.42  219.5475  +28.3817
  365  TXS 1435+285                      2.51e+03  5.0e+02       6.00   60148 0   -0.78    5.31  219.5413  +28.3633
  408  B2.2 1435+28                      1.89e+03  3.8e+02       0.00   60148 0   -0.78    5.31  219.5412  +28.3600
 1400  FIRST J143809.9+282146            8.32e+02  1.7e+02       5.00   60148 0   -0.78    5.31  219.5415  +28.3630
 1400  NVSS J143809+282147               8.21e+02  1.6e+02      45.00   60148 0   -0.78    5.31  219.5413  +28.3631
 1400  WB 1435+2834                      8.07e+02  1.6e+02     120.00   60148 0   -0.83    5.42  219.5400  +28.3578
 4850  87GB 143559.0+283433              2.32e+02  4.6e+01     138.00   60148 0   -0.78    5.31  219.5412  +28.3603
 4850  BWE 1435+2834                     2.18e+02  4.4e+01     138.00   60148 0   -0.78    5.31  219.5400  +28.3578
 4850  GB6 B1435+2834                    2.11e+02  4.2e+01     108.00   60148 0   -0.86    5.50  219.5442  +28.3608
 4850  MITG J143810+2822                 2.17e+02  4.3e+01     258.00   60148 0   -0.78    5.31  219.5446  +28.3697

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 +28.36                         3.60e+03  1.1e+03     690.00    60148  219.5475  +28.3817
   408  B2.2 1435+28                      1.89e+03  3.8e+02       0.00    60148  219.5412  +28.3600
  1400  FIRST J143810.5+282003            1.50e+00  3.0e-01       5.00   -60148  219.5438  +28.3343
  1400  FIRST J143815.6+282015            6.20e+00  1.2e+00       5.00   -60148  219.5654  +28.3375
  4850  GB6 B1435+2834                    2.11e+02  4.2e+01     108.00    60148  219.5442  +28.3608

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