Complement to VIII/85A

Source NVSS_J035015+700541: 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  6C 034507+695556                  6.50e+02  1.3e+02     252.00   99661 0   -0.50    3.91  057.5621  +70.0842
  325  WN B0345.1+6956                   4.70e+02  9.4e+01      12.00   99661 0   -0.50    3.91  057.5610  +70.0948
  365  TXS 0345+699                      6.59e+02  1.3e+02       6.00   99661 0   -0.68    4.56  057.5690  +70.0902
 1400  NVSS J035015+700541               2.08e+02  4.2e+01      45.00   99661 0   -0.50    3.91  057.5628  +70.0947
 1400  WB 0345+6956                      2.66e+02  5.3e+01     120.00   99661 0   -0.53    3.99  057.5642  +70.0872
 4850  87GB 034507.9+695605              1.13e+02  2.3e+01     138.00   99661 0   -0.50    3.91  057.5646  +70.0867
 4850  BWE 0345+6956                     8.70e+01  1.7e+01     138.00   99661 0   -0.56    4.08  057.5642  +70.0872
 4850  GB6 B0345+6956                    1.06e+02  2.1e+01     108.00   99661 0   -0.54    4.03  057.5696  +70.0872
 4850  IRAS F03451+6956                  9.20e+01  1.8e+01     210.00   99661 0   -0.51    3.93  057.5637  +70.0950

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  


   151  6C 034507+695556                  6.50e+02  1.3e+02     252.00    99661  057.5621  +70.0842
   232  MY 034507.3+700426.7              4.00e+02  8.0e+01     150.00   -99661  057.5617  +70.0741
   325  WN B0345.1+6956                   4.70e+02  9.4e+01      12.00    99661  057.5610  +70.0948
   365  TXS 0345+699                      6.59e+02  1.3e+02       6.00    99661  057.5690  +70.0902
  1400  NVSS J035015+700541               2.08e+02  4.2e+01      45.00    99661  057.5628  +70.0947
  1400  WB 0345+6956                      2.66e+02  5.3e+01     120.00    99661  057.5642  +70.0872
  4850  87GB 034507.9+695605              1.13e+02  2.3e+01     138.00    99661  057.5646  +70.0867

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