Complement to VIII/104

Source 7C_091345.39+654251.00: 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  


   38  8C 091343+654245                      3.50e+03  7.0e+02      270.0000  126429   -0.42     4.21  139.4708  +65.5025
   74  VLSSr J091756.2+653016                2.64e+03  5.3e+02       75.0000  126429   -0.64     4.71  139.4843  +65.5047
  150  TGSSADR J091755.6+653014              2.09e+03  4.2e+02       25.0020  126429   -0.64     4.71  139.4819  +65.5042
  151  6C 091345+654253                      3.07e+03  6.1e+02      252.0000  126429   -0.71     4.99  139.4812  +65.5047
  151  7C 091345.39+654251.00                2.08e+03  4.2e+02       70.2000  126429   -0.64     4.71  139.4829  +65.5042
  325  WN B0913.7+6542                       1.56e+03  3.1e+02       12.0000  126429   -0.64     4.71  139.4817  +65.5042
  365  TXS 0913+657                          1.35e+03  2.7e+02        6.0000  126429   -0.64     4.71  139.4831  +65.5041
 1400  NVSS J091755+653014                   6.23e+02  1.2e+02       45.0000  126429   -0.64     4.71  139.4821  +65.5040
 1400  WB 0913+6542                          6.09e+02  1.2e+02      120.0000  126429   -0.62     4.68  139.4829  +65.5036
 4850  87GB 091345.1+654249                  2.42e+02  4.8e+01      138.0000  126429   -0.62     4.67  139.4817  +65.5036
 4850  BWE 0913+6542                         2.39e+02  4.8e+01      138.0000  126429   -0.55     4.52  139.4829  +65.5036
 4850  GB6 B0913+6542                        2.26e+02  4.5e+01      108.0000  126429   -0.64     4.71  139.4796  +65.5025

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 J010921.9+043306           4.29e+01  8.6e+00       25.0020   -126429  017.3414  +04.5517
   200  GLEAM J010918+043436               1.55e+02  3.8e+01      120.0000   -126429  017.3275  +04.5769
  1400  NVSS J010922+043305                1.29e+01  2.6e+00       45.0000   -126429  017.3421  +04.5516

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