Complement to VIII/85A

Source CLASS_J161531.0981+213011.144: 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  


  365  TXS 1613+216                      2.82e+02  5.6e+01       6.00   68110 4   -0.09    2.68  243.8796  +21.5026
 1400  FIRST J161531.1+213011            2.14e+02  4.3e+01       5.00   68110 4   -0.09    2.68  243.8796  +21.5031
 1400  NVSS J161531+213011               2.49e+02  5.0e+01      45.00   68110 4   -0.09    2.67  243.8795  +21.5031
 1400  WB 1613+2137                      2.05e+02  4.1e+01     120.00   68110 4   -0.09    2.68  243.8796  +21.5008
 4850  87GB 161321.0+213728              2.60e+02  5.2e+01     138.00   68110 4   -0.09    2.69  243.8796  +21.5008
 4850  BWE 1613+2137                     2.02e+02  4.0e+01     138.00   68110 4   -0.13    2.78  243.8796  +21.5008
 4850  GB6 B1613+2137                    2.25e+02  4.5e+01     108.00   68110 4   -0.09    2.69  243.8771  +21.5008
 4850  MITG J161531+2130                 2.33e+02  4.7e+01     258.00   68110 4   -0.09    2.69  243.8812  +21.5022
 8400  CLASS J161531.0981+213011.144     2.12e+02  4.2e+01       0.33   68110 4   -0.09    2.67  243.8795  +21.5031
 8400  JVAS J1615+2130                   2.11e+02  4.2e+01       0.33   68110 4   -0.09    2.69  243.8796  +21.5031

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 J161531+213011               2.49e+02  5.0e+01      45.00    68110  243.8795  +21.5031
  1400  WB 1613+2137                      2.05e+02  4.1e+01     120.00    68110  243.8796  +21.5008
  4850  GB6 B1613+2137                    2.25e+02  4.5e+01     108.00    68110  243.8771  +21.5008
  8400  CLASS J161530.7273+213011.989     1.43e+01  2.9e+00       0.33   -68110  243.8780  +21.5033
  8400  CLASS J161530.9607+213016.437     7.50e+00  1.5e+00       0.33   -68110  243.8790  +21.5046
  8400  CLASS J161531.3042+213004.634     4.30e+00  9.0e-01       0.33   -68110  243.8804  +21.5013

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