Complement to VIII/85A

Source TXS_1708+006: 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 J1710.5+0036                 5.30e+03  1.1e+03      79.98   73646 5   -0.52    4.77  257.6467  +00.6100
  178  4C +00.65                         4.00e+03  1.2e+03     690.00   73646 5   -0.52    4.77  257.6467  +00.5850
  365  TXS 1708+006                      2.73e+03  5.5e+02       6.00   73646 5   -0.52    4.77  257.6470  +00.6095
  408  MRC 1708+006                      2.65e+03  5.3e+02     120.00   73646 5   -0.52    4.77  257.6463  +00.6081
 1400  NVSS J171035+003702               1.34e+03  2.7e+02      45.00   73646 5   -0.53    4.79  257.6473  +00.6172
 1400  WB 1708+0039                      1.36e+03  2.7e+02     120.00   73646 5   -0.52    4.76  257.6450  +00.6050
 4850  87GB 170801.6+003956              8.88e+02  1.8e+02     138.00   73646 5   -0.52    4.77  257.6446  +00.6044
 4850  BWE 1708+0039                     7.15e+02  1.4e+02     138.00   73646 5   -0.52    4.76  257.6450  +00.6050
 4850  GB6 B1708+0040                    7.09e+02  1.4e+02     108.00   73646 5   -0.52    4.76  257.6446  +00.6072
 4850  MITG J171036+0036                 5.48e+02  1.1e+02     258.00   73646 5   -0.52    4.76  257.6513  +00.6106
 4850  PMN J1710+0036                    5.82e+02  1.2e+02     168.00   73646 5   -0.56    4.86  257.6458  +00.6125

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  


   178  4C +00.65                         4.00e+03  1.2e+03     690.00    73646  257.6467  +00.5850
  1400  NVSS J171032+003510               7.60e+00  1.5e+00      45.00   -73646  257.6371  +00.5861
  1400  NVSS J171039+003509               7.00e+00  1.4e+00      45.00   -73646  257.6630  +00.5859
  4850  87GB 170801.6+003956              8.88e+02  1.8e+02     138.00    73646  257.6446  +00.6044
  4850  PMN J1710+0036                    5.82e+02  1.2e+02     168.00    73646  257.6458  +00.6125

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