Complement to VIII/85A

Source CLASS_J141035.0750+073121.481: 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  


 1400  FIRST J141035.0+073122            1.29e+02  2.6e+01       5.00   59254 0    0.53    0.43  212.6462  +07.5228
 1400  NVSS J141035+073121               1.92e+02  3.8e+01      45.00   59254 0    0.37    1.13  212.6463  +07.5225
 4850  87GB 140806.9+074514              4.60e+02  9.2e+01     138.00   59254 0    0.37    1.13  212.6496  +07.5186
 4850  BWE 1408+0745                     3.48e+02  7.0e+01     138.00   59254 0    0.31    1.31  212.6500  +07.5194
 4850  GB6 B1408+0745                    3.90e+02  7.8e+01     108.00   59254 0    0.31    1.31  212.6450  +07.5211
 4850  PMN J1410+0731                    3.03e+02  6.1e+01     168.00   59254 0    0.31    1.31  212.6458  +07.5225
 8400  CLASS J141035.0750+073121.481     3.35e+02  6.7e+01       0.33   59254 0    0.37    1.13  212.6461  +07.5226
 8400  JVAS J1410+0731                   3.32e+02  6.6e+01       0.33   59254 0    0.37    1.13  212.6461  +07.5226

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  


   365  TXS 1408+077                      1.39e+02  2.8e+01       6.00   -59254  212.6619  +07.5378
  1400  FIRST J141035.0+073122            1.28e+02  2.6e+01       5.00    59254  212.6462  +07.5228
  1400  NVSS J141035+073121               1.92e+02  3.8e+01      45.00    59254  212.6463  +07.5225
  4850  87GB 140806.9+074514              4.60e+02  9.2e+01     138.00    59254  212.6496  +07.5186
  4850  GB6 B1408+0745                    3.90e+02  7.8e+01     108.00    59254  212.6450  +07.5211
  4850  MITG J141035+0730                 1.74e+02  3.5e+01     258.00   -59254  212.6463  +07.5147
  4850  PMN J1410+0731                    3.03e+02  6.1e+01     168.00    59254  212.6458  +07.5225
  8400  CLASS J141035.0750+073121.481     3.35e+02  6.7e+01       0.33    59254  212.6461  +07.5226

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