Complement to VIII/85A

Source WISH_B1221.9-1835C: 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  


  325  WISH B1221.9-1835A                8.60e+01  1.7e+01      18.00   52500 3    0.22    1.39  186.1265  -18.7888
  325  WISH B1221.9-1835C                8.80e+01  1.8e+01      18.00   52500 3    0.21    1.42  186.1386  -18.8161
 1400  NVSS J122430-184704               1.60e+02  3.2e+01      45.00   52500 3    0.21    1.42  186.1282  -18.7844
 4850  PMN J1224-1847                    1.55e+02  3.1e+01     168.00   52500 3    0.21    1.42  186.1337  -18.7844
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%