Complement to VIII/104

Source WISH_B0000.4-1628: 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  


   74  VLSSr J000310.0-161503                2.38e+03  4.8e+02       75.0000    3950   -0.65     4.65  000.7920  -16.2510
  150  TGSSADR J000310.1-161507              1.45e+03  2.9e+02       25.0020    3950   -0.65     4.65  000.7923  -16.2522
  182  KGS J000310-161506                    1.59e+03  3.2e+02        2.4000    3950   -0.63     4.55  000.7923  -16.2517
  200  GLEAM J000310-161503                  1.27e+03  2.5e+02      120.0000    3950   -0.65     4.65  000.7925  -16.2511
  325  WISH B0000.6-1631                     1.06e+03  2.1e+02       18.0000    3950   -0.65     4.65  000.7925  -16.2520
  365  TXS 0000-165                          9.81e+02  2.0e+02        6.0000    3950   -0.63     4.55  000.7933  -16.2519
  408  MRC 0000-165                          1.08e+03  2.2e+02      120.0000    3950   -0.65     4.65  000.7925  -16.2528
 1400  NVSS J000310-161506                   3.84e+02  7.7e+01       45.0000    3950   -0.65     4.65  000.7926  -16.2518
 2307  SPASS J000313-161552                  1.82e+02  3.6e+01      645.0000    3950   -0.67     4.61  000.8062  -16.2646
 2700  PKS J0003-1615                        2.50e+02  5.0e+01       60.0000    3950   -0.65     4.65  000.7963  -16.2528
 4850  PMN J0003-1615                        1.49e+02  3.0e+01      168.0000    3950   -0.65     4.65  000.7867  -16.2522

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  


   200  GLEAM J000255-161129               5.82e+01  1.2e+01      120.0000     -3950  000.7329  -16.1916
   325  WISH B0000.4-1628                  2.50e+01  5.0e+00       18.0000     -3950  000.7412  -16.1920
  1400  NVSS J000257-161128                1.02e+01  2.0e+00       45.0000     -3950  000.7406  -16.1912
  4850  PMN J0003-1615                     1.49e+02  3.0e+01      168.0000      3950  000.7867  -16.2522

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