Complement to VIII/85A

Source PMN_J0454-6911: 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  


  843  SUMSS J045403-691155              3.02e+02  6.0e+01      18.00   19639 0    0.21    1.93  073.5151  -69.1986
 2450  [FHW95]b LMCB0454-6916            7.88e+02  1.6e+02     531.00   19639 0   -0.07    2.97  073.5154  -69.1992
 2700  PKS J0454-6911                    4.50e+02  9.0e+01      60.00   19639 0   -0.08    2.99  073.5308  -69.1850
 4750  [FHW95]c LMCB0454-6916            5.44e+02  1.1e+02     288.00   19639 0    0.19    2.00  073.5258  -69.1914
 4850  PMN J0454-6911                    5.03e+02  1.0e+02     168.00   19639 0    0.19    2.00  073.5271  -69.1908
 8550  [FHW95]d LMCB0454-6916            4.59e+02  9.2e+01     162.00   19639 0    0.19    2.00  073.5450  -69.1875

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  


   843  SUMSS J045304-691216              1.10e+01  2.2e+00      18.00   -19639  073.2675  -69.2045
   843  SUMSS J045358-691036              1.00e+02  2.0e+01      18.00   -19639  073.4938  -69.1769
   843  SUMSS J045403-691155              3.02e+02  6.0e+01      18.00    19639  073.5151  -69.1986
   843  SUMSS J045425-691044              1.26e+02  2.5e+01      18.00   -19639  073.6050  -69.1791
   843  SUMSS J045506-691658              8.90e+00  1.8e+00      18.00   -19639  073.7756  -69.2829
  1400  [FHW95]a LMCB0454-6916            5.33e+02  1.1e+02     912.00   -19639  073.6112  -69.2047
  2450  [FHW95]b LMCB0454-6916            7.88e+02  1.6e+02     531.00    19639  073.5154  -69.1992
  2700  PKS J0454-6911                    4.50e+02  9.0e+01      60.00    19639  073.5308  -69.1850
  4750  [FHW95]c LMCB0454-6916            5.44e+02  1.1e+02     288.00    19639  073.5258  -69.1914
  4850  PMN J0454-6911                    5.03e+02  1.0e+02     168.00    19639  073.5271  -69.1908
  8550  [FHW95]d LMCB0454-6916            4.59e+02  9.2e+01     162.00    19639  073.5450  -69.1875

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