Complement to VIII/85A

Source WN_B1807.9+6604: 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  


  151  7C 180759.60+660453.00            1.58e+02  3.2e+01      70.20   79849 0   -0.96    4.28  272.0113  +66.0911
  325  WN B1807.9+6604                   6.80e+01  1.4e+01      12.00   79849 0   -0.92    4.19  272.0074  +66.0918
 1400  NVSS J180802+660530               2.05e+01  4.1e+00      45.00   79849 0   -0.96    4.28  272.0099  +66.0917
 1490  VLA-NEP J1808.1+6605              1.77e+01  3.5e+00      19.98   79849 0   -0.96    4.28  272.0160  +66.0926
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%