Complement to VIII/85A

Source FIRST_J081622.7+573909: 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 081218+574825                  2.30e+02  4.6e+01     252.00   32919 0   -0.34    3.09  124.0837  +57.6531
  151  7C 081220.30+574820.00            2.56e+02  5.4e+01      70.20   32919 0   -0.37    3.16  124.0925  +57.6517
  325  WN B0812.3+5748                   1.54e+02  3.1e+01      12.00   32919 0   -0.37    3.16  124.0936  +57.6528
 1400  FIRST J081622.7+573909            1.26e+02  2.5e+01       5.00   32919 0   -0.34    3.09  124.0947  +57.6525
 1400  NVSS J081622+573909               9.95e+01  2.0e+01      45.00   32919 0   -0.28    2.90  124.0945  +57.6526
 4850  87GB 081222.1+574811              9.86e+01  2.0e+01     138.00   32919 0   -0.37    3.16  124.0996  +57.6492
 4850  BWE 0812+5748                     6.40e+01  1.3e+01     138.00   32919 0   -0.37    3.17  124.1000  +57.6494
 4850  GB6 B0812+5748                    7.17e+01  1.4e+01     108.00   32919 0   -0.37    3.16  124.0950  +57.6494
 4885  RGB 0816+576                      6.40e+01  1.3e+01       4.02   32919 0   -0.37    3.16  124.0947  +57.6526

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 081218+574825                  2.30e+02  4.6e+01     252.00    32919  124.0837  +57.6531
  1400  FIRST J081622.6+573854            4.50e+00  9.0e-01       5.00   -32919  124.0943  +57.6485
  1400  NVSS J081622+573909               9.95e+01  2.0e+01      45.00    32919  124.0945  +57.6526
  4850  87GB 081222.1+574811              9.86e+01  2.0e+01     138.00    32919  124.0996  +57.6492
  4850  BWE 0812+5748                     6.40e+01  1.3e+01     138.00    32919  124.1000  +57.6494
  4850  GB6 B0812+5748                    7.17e+01  1.4e+01     108.00    32919  124.0950  +57.6494
  8400  CLASS J081623.8222+573909.509     9.20e+01  1.8e+01       0.33   -32919  124.0993  +57.6526

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