Complement to VIII/85A

Source SUMSS_J050529-665557: 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 J050529-665557              1.54e+02  3.1e+01      18.00   19680 0   -0.21    2.81  076.3734  -66.9325
 2450  [FHW95]b LMCB0505-6659            1.27e+02  2.5e+01     531.00   19680 0   -0.21    2.81  076.3062  -66.9419
 4750  [FHW95]c LMCB0505-6659            1.07e+02  2.1e+01     288.00   19680 0   -0.21    2.81  076.3538  -66.9283
 4850  PMN J0505-6655                    7.80e+01  1.6e+01     168.00   19680 0   -0.25    2.92  076.3483  -66.9269
 8550  [FHW95]d LMCB0505-6659            9.40e+01  1.9e+01     162.00   19680 0   -0.21    2.81  076.3492  -66.9275

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 J050409-670111              1.06e+02  2.1e+01      18.00   -19680  076.0401  -67.0199
   843  SUMSS J050430-670222              7.30e+00  1.5e+00      18.00   -19680  076.1253  -67.0395
   843  SUMSS J050452-670123              3.95e+01  7.9e+00      18.00   -19680  076.2182  -67.0232
   843  SUMSS J050520-665507              3.03e+01  6.1e+00      18.00   -19680  076.3350  -66.9189
   843  SUMSS J050529-665557              1.54e+02  3.1e+01      18.00    19680  076.3734  -66.9325
   843  SUMSS J050543-665814              2.92e+01  5.8e+00      18.00   -19680  076.4295  -66.9708
   843  SUMSS J050553-665941              7.20e+00  1.4e+00      18.00   -19680  076.4735  -66.9947
  1400  [FHW95]a LMCB0505-6659            1.38e+02  2.8e+01     912.00   -19680  076.2442  -66.9467
  2450  [FHW95]b LMCB0505-6659            1.27e+02  2.5e+01     531.00    19680  076.3062  -66.9419
  4750  [FHW95]c LMCB0505-6659            1.07e+02  2.1e+01     288.00    19680  076.3538  -66.9283
  4850  PMN J0505-6655                    7.80e+01  1.6e+01     168.00    19680  076.3483  -66.9269
  8550  [FHW95]d LMCB0505-6659            9.40e+01  1.9e+01     162.00    19680  076.3492  -66.9275

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