Complement to VIII/85A

Source NVSS_J231933-093601: 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 J2319.5-0936                 1.30e+03  2.6e+02      79.98   97895 4   -0.83    4.67  349.8850  -09.6010
  325  WISH B2316.9-0952                 3.36e+02  6.7e+01      18.00   97895 4   -0.82    4.64  349.8885  -09.5937
 1400  FIRST J231933.2-093557            6.26e+01  1.3e+01       5.00   97895 4   -1.03    5.05  349.8886  -09.5994
 1400  NVSS J231933-093601               1.12e+02  2.2e+01      45.00   97895 4   -0.82    4.64  349.8886  -09.6003
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
No object found

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