Complement to VIII/104

Source VIPS_J10248+2332: 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  


  150  TGSSADR J102453.6+233234              6.76e+01  1.4e+01       25.0020  142477    0.21     1.37  156.2237  +23.5429
  200  GLEAM J102452+233217                  1.63e+02  3.3e+01      120.0000  142477    0.16     1.48  156.2194  +23.5381
 1400  FIRST14 J102453.6+233234              1.25e+02  2.5e+01        4.9998  142477   -0.06     2.36  156.2234  +23.5428
 1400  NVSS J102453+233233                   1.09e+02  2.2e+01       45.0000  142477    0.16     1.48  156.2233  +23.5427
 1400  WB 1022+2347                          1.32e+02  2.6e+01      120.0000  142477   -0.07     2.38  156.2342  +23.5372
 4850  87GB 102210.2+234727                  1.68e+02  3.4e+01      138.0000  142477    0.16     1.48  156.2329  +23.5369
 4850  BWE 1022+2347                         1.30e+02  2.6e+01      138.0000  142477    0.19     1.42  156.2342  +23.5372
 4850  GB6 B1022+2347                        1.63e+02  3.3e+01      108.0000  142477    0.16     1.48  156.2250  +23.5419
 4850  MITG J102456+2332                     1.82e+02  3.6e+01      258.0000  142477    0.21     1.37  156.2350  +23.5389
 5000  VIPS J10248+2332                      1.05e+02  2.1e+01        0.0009  142477    0.16     1.48  156.2235  +23.5428
 8400  CLASS J102453.6394+233233.960         1.28e+02  2.6e+01        0.3300  142477    0.16     1.48  156.2235  +23.5428
 8400  CRATES J102454+233231                 1.28e+02  2.6e+01        6.0000  142477    0.01     2.05  156.2235  +23.5428

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  


   325  WN B0132.3+4856                    3.00e+01  6.0e+00       12.0000   -142477  023.8500  +49.2021
  1400  NVSS J013524+491200                1.33e+01  2.7e+00       45.0000   -142477  023.8522  +49.2000
  4850  GB6 B0132+4857                     2.88e+01  5.8e+00      108.0000   -142477  023.8333  +49.2117

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