Complement to VIII/85A

Source TXS_1358-065: 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 J1400.8-0645                 8.50e+03  1.7e+03      79.98   62117 0   -1.12    6.02  210.2192  -06.7621
  365  TXS 1358-065                      1.86e+03  3.7e+02       6.00   62117 0   -1.11    6.01  210.2189  -06.7616
  408  MRC 1358-065                      1.53e+03  3.1e+02     120.00   62117 0   -1.12    6.02  210.2188  -06.7617
 1400  FIRST J140052.4-064545            1.89e+02  3.8e+01       5.00   62117 0   -1.29    6.35  210.2185  -06.7626
 1400  NVSS J140052-064541               3.19e+02  6.4e+01      45.00   62117 0   -1.11    6.01  210.2186  -06.7615

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  


    74  VLSS J1400.8-0645                 8.50e+03  1.7e+03      79.98    62117  210.2192  -06.7621
   178  4C -06.36                         3.20e+03  9.6e+02     690.00   -62117  210.2108  -06.7367
   365  TXS 1358-065                      1.86e+03  3.7e+02       6.00    62117  210.2189  -06.7616
   408  MRC 1358-065                      1.53e+03  3.1e+02     120.00    62117  210.2188  -06.7617
  1400  FIRST J140046.4-064928            7.40e+00  1.5e+00       5.00   -62117  210.1937  -06.8246
  1400  FIRST J140047.1-064924            1.60e+00  3.0e-01       5.00   -62117  210.1965  -06.8236
  1400  FIRST J140049.7-064919            2.90e+00  6.0e-01       5.00   -62117  210.2072  -06.8221
  1400  FIRST J140052.4-064545            1.89e+02  3.8e+01       5.00    62117  210.2185  -06.7626
  1400  FIRST J140052.6-064536            1.38e+02  2.8e+01       5.00   -62117  210.2195  -06.7601
  1400  NVSS J140047-064927               1.61e+01  3.2e+00      45.00   -62117  210.1968  -06.8244
  1400  NVSS J140048-064302               2.30e+00  5.0e-01      45.00   -62117  210.2040  -06.7173
  1400  NVSS J140052-064541               3.19e+02  6.4e+01      45.00    62117  210.2186  -06.7615

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