Complement to VIII/85A

Source PMN_J0703-0930a: 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 J0703.1-0929                 8.50e+02  1.7e+02      79.98   27486 0   -0.56    3.97  105.7862  -09.4977
  365  TXS 0700-094                      4.19e+02  8.4e+01       6.00   27486 0   -0.56    3.97  105.7869  -09.4991
 1400  NVSS J070308-092956               1.59e+02  3.2e+01      45.00   27486 0   -0.56    3.97  105.7860  -09.4990
 2700  F3R 6043                          1.20e+02  3.2e+01     150.00   27486 0   -0.54    3.95  105.7892  -09.4942
 4850  PMN J0703-0929                    8.30e+01  1.7e+01     168.00   27486 0   -0.56    3.97  105.7938  -09.4958
 4850  PMN J0703-0930a                   1.02e+02  2.0e+01     168.00   27486 0   -0.54    3.95  105.8008  -09.5047

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 J0703.1-0929                 8.50e+02  1.7e+02      79.98    27486  105.7862  -09.4977
   365  TXS 0700-094                      4.19e+02  8.4e+01       6.00    27486  105.7869  -09.4991
  1400  NVSS J070305-092401               6.40e+00  1.3e+00      45.00   -27486  105.7743  -09.4003
  1400  NVSS J070308-092956               1.59e+02  3.2e+01      45.00    27486  105.7860  -09.4990
  1400  NVSS J070330-092553               4.70e+00  9.0e-01      45.00   -27486  105.8752  -09.4316
  1400  NVSS J070330-093519               2.60e+00  5.0e-01      45.00   -27486  105.8754  -09.5889
  1410  RRF 2459                          4.07e+02  8.1e+01     564.00   -27486  105.8133  -09.4861
  2700  F3R 6043                          1.20e+02  3.2e+01     150.00    27486  105.7892  -09.4942
  4850  PMN J0703-0925                    4.80e+01  1.1e+01     168.00   -27486  105.8771  -09.4217
  4850  PMN J0703-0929                    8.30e+01  1.7e+01     168.00    27486  105.7938  -09.4958
  4850  PMN J0703-0930b                   7.20e+01  1.4e+01     168.00   -27486  105.9017  -09.5069

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