Complement to VIII/104

Source PKS_J0922-3959: 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 1 column 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/104/spectra
Post annotation 		SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
2021A&A...655A..17S

The parameters of the radio spectra[image] (1658207 rows)		img(gal)
start AladinLite 
  nu   Name                                   S(nu)       e         beam        Seq      a       b      RAJ2000   DEJ2000
 MHz                                           mJy       mJy       arcsec                      [mJy]      deg       deg  


   80  Cula 0920-397                         1.20e+04  2.4e+03      222.0000  128588   -0.50     4.98  140.6912  -39.9844
  150  TGSSADR J092246.2-395936              7.93e+03  1.6e+03       25.0020  128588   -0.46     4.90  140.6928  -39.9933
  160  Culb 0920-397                         8.00e+03  1.6e+03      111.0000  128588   -0.52     5.04  140.6912  -39.9844
  408  MRC 0920-397                          4.38e+03  8.8e+02      120.0000  128588   -0.46     4.90  140.6933  -39.9936
  843  MGPS J092246-395935                   3.16e+03  6.3e+02       45.0000  128588   -0.46     4.90  140.6928  -39.9931
 1400  NVSS J092246-395934                   2.61e+03  5.2e+02       45.0000  128588   -0.46     4.90  140.6932  -39.9928
 2700  PKS J0922-3959                        1.60e+03  3.2e+02       60.0000  128588   -0.32     4.41  140.6933  -39.9931
 4800  ATPMN5 J092246.42-395934              1.39e+03  2.8e+02        1.8000  128588   -0.50     4.98  140.6935  -39.9930
 4850  PMN J0922-3959                        1.89e+03  3.8e+02      168.0000  128588   -0.46     4.90  140.6887  -39.9892
 8400  ATPMN8 J092246.42-395934              1.24e+03  2.5e+02        1.2000  128588   -0.50     4.98  140.6935  -39.9930
 8400  [PK2012]8IVS 0920-397                 1.12e+03  2.2e+02        0.0020  128588   -0.50     4.98  140.6934  -39.9931
 8400  PKS8400 J0922-3959                    1.65e+03  3.3e+02      162.0000  128588   -0.46     4.90  140.6934  -39.9931

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/104/waste
Post annotation 		SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
2021A&A...655A..17S

Source parameters based on positional cross-id[spectrum] (3570814 rows)		img(gal)
start AladinLite 
  nu    Name                                S(nu)       e         beam         Seq     RAJ2000   DEJ2000
  MHz                                        mJy       mJy       arcsec                  deg       deg  


   150  TGSSADR J001140.6-490014           3.21e+01  6.4e+00       25.0020   -128588  002.9194  -49.0039
   200  GLEAM J001137-490056               8.08e+01  1.6e+01      120.0000   -128588  002.9075  -49.0157
   843  SUMSS J001141-490014               1.56e+01  3.1e+00       18.0000   -128588  002.9210  -49.0039

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