Complement to VIII/85A

Source NVSS_J001946+654520: 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 J0019.7+6545                 3.08e+03  6.2e+02      79.98     688 0   -0.92    5.21  004.9477  +65.7533
  325  WN B0017.0+6528                   8.67e+02  1.7e+02      12.00     688 0   -0.92    5.21  004.9428  +65.7565
  365  TXS 0017+654                      7.14e+02  1.4e+02       6.00     688 0   -0.92    5.21  004.9436  +65.7562
 1400  NVSS J001946+654520               2.08e+02  4.2e+01      45.00     688 0   -0.92    5.21  004.9427  +65.7558
 1410  RRF 1166                          1.41e+02  2.8e+01     564.00     688 0   -0.90    5.03  004.9508  +65.7611
 2700  F3R 3617                          1.20e+02  3.2e+01     150.00     688 0   -0.92    5.21  004.9562  +65.7514
 4850  87GB 001700.3+652826              5.50e+01  1.1e+01     138.00     688 0   -0.92    5.21  004.9413  +65.7514
 4850  BWE 0017+6528                     5.30e+01  1.1e+01     138.00     688 0   -0.92    5.21  004.9433  +65.7508
 4850  GB6 B0017+6528                    5.60e+01  1.1e+01     108.00     688 0   -0.92    5.21  004.9429  +65.7531

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  


    74  VLSS J0019.7+6545                 3.08e+03  6.2e+02      79.98      688  004.9477  +65.7533
   232  MY 001700.5+654526.5              4.50e+02  1.1e+02     150.00     -688  004.9421  +65.7574
   325  WN B0017.0+6528                   8.67e+02  1.7e+02      12.00      688  004.9428  +65.7565
   365  TXS 0017+654                      7.14e+02  1.4e+02       6.00      688  004.9436  +65.7562
  1400  NVSS J001946+654520               2.08e+02  4.2e+01      45.00      688  004.9427  +65.7558
  2700  F3R 3617                          1.20e+02  3.2e+01     150.00      688  004.9562  +65.7514
  4850  BWE 0017+6528                     5.30e+01  1.1e+01     138.00      688  004.9433  +65.7508

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