Complement to VIII/85A

Source TXS_0358+539: 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 J0402.5+5404                 5.20e+02  1.0e+02      79.98   16163 0   -0.55    3.74  060.6262  +54.0692
  151  6C 035841+535531                  3.50e+02  7.0e+01     252.00   16163 0   -0.55    3.74  060.6475  +54.0639
  232  MY 035840.5+540411.4              1.80e+02  4.7e+01     150.00   16163 0   -0.49    3.55  060.6417  +54.0698
  325  WN B0358.6+5355                   2.55e+02  5.1e+01      12.00   16163 0   -0.55    3.74  060.6348  +54.0692
  365  TXS 0358+539                      2.88e+02  5.8e+01       6.00   16163 0   -0.55    3.74  060.6327  +54.0698
 1400  NVSS J040232+540411               1.00e+02  2.0e+01      45.00   16163 0   -0.55    3.74  060.6337  +54.0697
 1410  RRF 1548                          1.04e+02  2.1e+01     564.00   16163 0   -0.55    3.74  060.6779  +54.0606
 2700  F3R 4331                          7.00e+01  1.4e+01     150.00   16163 0   -0.55    3.74  060.6354  +54.0611
 4850  87GB 035839.2+535536              6.96e+01  1.4e+01     138.00   16163 0   -0.55    3.74  060.6362  +54.0653
 4850  BWE 0358+5355                     5.80e+01  1.2e+01     138.00   16163 0   -0.55    3.74  060.6379  +54.0639
 4850  GB6 B0358+5355                    5.20e+01  1.0e+01     108.00   16163 0   -0.55    3.75  060.6371  +54.0633

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 035841+535531                  3.50e+02  7.0e+01     252.00    16163  060.6475  +54.0639
   325  WN B0358.5+5352                   3.20e+01  6.4e+00      12.00   -16163  060.6029  +54.0179
  1400  NVSS J040224+540100               7.50e+00  1.5e+00      45.00   -16163  060.6017  +54.0168
  1400  NVSS J040246+540330               3.90e+00  8.0e-01      45.00   -16163  060.6938  +54.0584
  1410  RRF 1548                          1.04e+02  2.1e+01     564.00    16163  060.6779  +54.0606

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