Complement to VIII/85A

Source BWE_1714+5600: 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 171430+560118                  5.30e+02  1.1e+02     252.00   73806 0   -0.79    4.50  258.8646  +55.9675
  151  7C 171430.89+560109.00            5.76e+02  1.2e+02      70.20   73806 0   -0.80    4.56  258.8645  +55.9647
  325  WN B1714.5+5601                   3.68e+02  7.4e+01      12.00   73806 0   -0.80    4.56  258.8655  +55.9652
  365  TXS 1714+560                      3.05e+02  6.1e+01       6.00   73806 0   -0.79    4.51  258.8646  +55.9650
 1400  FIRST J171527.7+555754            1.18e+02  2.4e+01       5.00   73806 0   -0.79    4.51  258.8655  +55.9653
 1400  NVSS J171527+555755               1.19e+02  2.4e+01      45.00   73806 0   -0.79    4.50  258.8657  +55.9653
 1400  WB 1714+5600                      1.18e+02  2.4e+01     120.00   73806 0   -0.76    4.42  258.8637  +55.9619
 4850  87GB 171429.4+560100              4.00e+01  8.0e+00     138.00   73806 0   -0.79    4.50  258.8587  +55.9622
 4850  BWE 1714+5600                     4.30e+01  8.6e+00     138.00   73806 0   -0.79    4.51  258.8637  +55.9619
 4850  GB6 B1714+5600                    3.80e+01  7.6e+00     108.00   73806 0   -0.81    4.55  258.8600  +55.9619

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 171430+560118                  5.30e+02  1.1e+02     252.00    73806  258.8646  +55.9675
   232  MY 171429.8+555747.4              2.30e+02  5.2e+01     150.00   -73806  258.8604  +55.9632
   325  WN B1714.5+5601                   3.68e+02  7.4e+01      12.00    73806  258.8655  +55.9652
   365  TXS 1714+560                      3.05e+02  6.1e+01       6.00    73806  258.8646  +55.9650
  1400  WB 1714+5600                      1.18e+02  2.4e+01     120.00    73806  258.8637  +55.9619
  4850  87GB 171429.4+560100              4.00e+01  8.0e+00     138.00    73806  258.8587  +55.9622

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