Complement to VIII/85A

Source WB_0801+0429: 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  


  611  NAIC 0801+045                     4.51e+02  9.0e+01     756.00   32448 0   -0.26    3.37  120.9933  +04.3775
 1400  NVSS J080356+042102               3.18e+02  6.4e+01      45.00   32448 0   -0.26    3.37  120.9853  +04.3508
 1400  WB 0801+0429                      3.26e+02  6.5e+01     120.00   32448 0   -0.30    3.50  120.9850  +04.3486
 4775  NAICGB 0801+044                   2.00e+02  4.0e+01     168.00   32448 0   -0.25    3.30  120.9867  +04.3536
 4850  87GB 080118.2+042926              2.87e+02  5.7e+01     138.00   32448 0   -0.26    3.37  120.9850  +04.3486
 4850  BWE 0801+0429                     2.41e+02  4.8e+01     138.00   32448 0   -0.30    3.50  120.9850  +04.3486
 4850  GB6 B0801+0429                    2.81e+02  5.6e+01     108.00   32448 0   -0.26    3.37  120.9854  +04.3528
 4850  MITG J080357+0420                 2.92e+02  5.8e+01     258.00   32448 0   -0.20    3.13  120.9900  +04.3500
 4850  PMN J0803+0421                    2.98e+02  6.0e+01     168.00   32448 0   -0.26    3.37  120.9846  +04.3508
 8400  CLASS J080356.4429+042102.721     2.30e+02  4.6e+01       0.33   32448 0   -0.26    3.37  120.9852  +04.3508
 8400  JVAS J0803+0421                   2.42e+02  4.8e+01       0.33   32448 0   -0.24    3.32  120.9852  +04.3508

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  


   611  NAIC 0801+045                     4.51e+02  9.0e+01     756.00    32448  120.9933  +04.3775
  1400  NVSS J080343+042156               1.98e+01  4.0e+00      45.00   -32448  120.9300  +04.3657
  1400  NVSS J080403+042222               6.83e+01  1.4e+01      45.00   -32448  121.0135  +04.3729
  1400  NVSS J080403+042346               3.40e+00  7.0e-01      45.00   -32448  121.0135  +04.3963
  4850  PMN J0803+0421                    2.98e+02  6.0e+01     168.00    32448  120.9846  +04.3508

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