Complement to VIII/85A

Source JVAS_J1855+377: 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  


  325  WN B1853.7+3738                   1.47e+02  2.9e+01      12.00   85087 5    0.13    1.84  283.8648  +37.7156
 1400  NVSS J185527+374256               1.87e+02  3.7e+01      45.00   85087 5    0.13    1.84  283.8652  +37.7156
 8400  CLASS J185527.7106+374256.993     2.28e+02  4.6e+01       0.33   85087 5    0.13    1.83  283.8655  +37.7158
 8400  JVAS J1855+377                    2.22e+02  4.4e+01       0.33   85087 5    0.13    1.84  283.8654  +37.7158

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  


   325  WN B1853.7+3738                   1.47e+02  2.9e+01      12.00    85087  283.8648  +37.7156
   325  WN B1853.8+3738                   2.60e+01  5.2e+00      12.00   -85087  283.9058  +37.7103
   365  TXS 1853+376                      2.09e+02  4.2e+01       6.00   -85087  283.8482  +37.7300
   408  B3 1853+376                       2.80e+02  5.6e+01      84.00   -85087  283.8662  +37.7200
  1400  NVSS J185527+374256               1.87e+02  3.7e+01      45.00    85087  283.8652  +37.7156
  1400  NVSS J185537+374242               9.60e+00  1.9e+00      45.00   -85087  283.9061  +37.7118
  1400  WB 1853+3738                      3.14e+02  6.3e+01     120.00   -85087  283.8696  +37.7089
  4850  87GB 185345.0+373835              4.19e+02  8.4e+01     138.00   -85087  283.8696  +37.7089
  4850  GB6 B1853+3738                    3.67e+02  7.3e+01     108.00   -85087  283.8675  +37.7128
  4850  MITG J185528+3742                 2.10e+02  4.2e+01     258.00   -85087  283.8679  +37.7142
  4850  MITG J185529+3742                 4.21e+02  8.4e+01     258.00   -85087  283.8729  +37.7147
  4850  MITG J185530+3743                 3.96e+02  7.9e+01     258.00   -85087  283.8775  +37.7233
  8400  JVAS J1855+377                    2.22e+02  4.4e+01       0.33    85087  283.8654  +37.7158

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