Complement to VIII/85A

Source NVSS_J090120+195205: 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 J0901.3+1952                 5.58e+03  1.1e+03      79.98   34462 5   -0.83    5.29  135.3350  +19.8677
  178  4C +19.32                         2.70e+03  8.1e+02     690.00   34462 5   -0.82    5.28  135.3392  +19.8017
  365  TXS 0858+200                      1.67e+03  3.3e+02       6.00   34462 5   -0.81    5.26  135.3353  +19.8679
 1400  FIRST J090120.4+195204            5.14e+02  1.0e+02       5.00   34462 5   -0.81    5.26  135.3353  +19.8679
 1400  NVSS J090120+195205               5.31e+02  1.1e+02      45.00   34462 5   -0.81    5.26  135.3353  +19.8681
 1400  WB 0858+2003                      4.89e+02  9.8e+01     120.00   34462 5   -0.82    5.28  135.3371  +19.8697
 2700  PKS J0901+1952                    2.90e+02  5.8e+01      60.00   34462 5   -0.82    5.28  135.3304  +19.8689
 4850  87GB 085829.9+200358              2.19e+02  4.4e+01     138.00   34462 5   -0.81    5.26  135.3367  +19.8694
 4850  BWE 0858+2003                     2.14e+02  4.3e+01     138.00   34462 5   -0.82    5.28  135.3371  +19.8697
 4850  GB6 B0858+2003                    2.17e+02  4.3e+01     108.00   34462 5   -0.82    5.28  135.3354  +19.8683
 4850  MITG J090123+1952                 1.68e+02  3.4e+01     258.00   34462 5   -0.82    5.28  135.3462  +19.8811

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 +19.32                         2.70e+03  8.1e+02     690.00    34462  135.3392  +19.8017
  1400  FIRST J090120.7+195304            4.48e+01  9.0e+00       5.00   -34462  135.3365  +19.8846
  1400  NVSS J090120+195311               3.18e+01  6.4e+00      45.00   -34462  135.3364  +19.8866
  4850  GB6 B0858+2003                    2.17e+02  4.3e+01     108.00    34462  135.3354  +19.8683
  4850  MITG J090123+1952                 1.68e+02  3.4e+01     258.00    34462  135.3462  +19.8811

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