Complement to VIII/85A

Source 5C13_121: 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="

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
No object foundThe 1 column 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/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  


   408  5C13 121                          6.29e+01  1.3e+01      90.00  -222305  240.4193  +43.2795
  1400  NVSS J160140+431647               7.59e+01  1.5e+01      45.00  -222305  240.4186  +43.2799
  4850  GB6 B1559+4325                    3.50e+01  7.0e+00     108.00  -222305  240.4087  +43.2878
  8400  CLASS J160140.7034+431658.844     8.00e-01  2.0e-01       0.33  -222305  240.4196  +43.2830
 15000  9C J1601+4316                     4.20e+01  8.4e+00      25.20  -222305  240.4187  +43.2800

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