Complement to VIII/85A

Source PKS_J1504+1029: 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  


  365  TXS 1502+106                      1.39e+03  2.8e+02       6.00  106705 4    0.06    3.04  226.1043  +10.4941
  408  MRC 1502+106                      1.55e+03  3.1e+02     120.00  106705 4    0.06    3.04  226.1046  +10.4953
 1400  FIRST J150424.9+102938            1.75e+03  3.5e+02       5.00  106705 4    0.06    3.03  226.1041  +10.4941
 1400  NVSS J150425+102938               1.77e+03  3.5e+02      45.00  106705 4    0.06    3.03  226.1043  +10.4940
 1400  WB 1501+1041                      1.55e+03  3.1e+02     120.00  106705 4    0.11    2.85  226.0979  +10.4928
 2700  PKS J1504+1029                    1.74e+03  3.5e+02      60.00  106705 4    0.06    3.04  226.1037  +10.4942
 4850  87GB 150158.6+104114              2.34e+03  4.7e+02     138.00  106705 4    0.06    3.03  226.0975  +10.4931
 4850  BWE 1501+1041                     2.33e+03  4.7e+02     138.00  106705 4    0.06    3.03  226.0979  +10.4928
 4850  GB6 B1501+1041                    2.32e+03  4.6e+02     108.00  106705 4    0.06    3.03  226.1000  +10.4953
 4850  MITG J150425+1028                 1.79e+03  3.6e+02     258.00  106705 4    0.06    3.04  226.1067  +10.4825
 8400  JVAS J1504+1029                   1.71e+03  3.4e+02       0.33  106705 4    0.06    3.04  226.1041  +10.4942

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 J1504.4+1029                 1.22e+03  2.4e+02      79.98  -106705  226.1054  +10.4955
   408  MRC 1502+106                      1.55e+03  3.1e+02     120.00   106705  226.1046  +10.4953
  1400  FIRST J150425.5+103010            2.10e+00  4.0e-01       5.00  -106705  226.1064  +10.5030
  4850  87GB 150158.6+104114              2.34e+03  4.7e+02     138.00   106705  226.0975  +10.4931
  4850  MITG J150425+1028                 1.79e+03  3.6e+02     258.00   106705  226.1067  +10.4825

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