Complement to VIII/104

Source TGSSADR_J012337.9+331536: 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  


  232  MY 012050.8+331509.7                  7.00e+02  1.4e+02      150.0000   30530   -1.22     5.67  020.9163  +33.2527
  325  WN B0120.8+3259A                      4.27e+02  8.5e+01       12.0000   30530   -1.22     5.67  020.9079  +33.2598
 1400  NVSS J012337+331534                   6.17e+01  1.2e+01       45.0000   30530   -1.22     5.67  020.9083  +33.2594
 2380  UGC 938                               3.50e+01  7.0e+00      162.0000   30530   -1.22     5.67  020.9167  +33.2561

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  


    74  VLSSr J012339.0+331526             1.28e+03  2.6e+02       75.0000    -30530  020.9125  +33.2573
   150  TGSSADR J012337.9+331536           8.45e+02  1.7e+02       25.0020    -30530  020.9081  +33.2602
   150  TGSSADR J012343.7+331449           4.76e+02  9.5e+01       25.0020    -30530  020.9322  +33.2471
   151  6Ca J012339+331508                 1.87e+03  3.7e+02      252.0000    -30530  020.9136  +33.2523
   232  MY 012050.8+331509.7               7.00e+02  1.4e+02      150.0000     30530  020.9163  +33.2527
   325  WN B0120.8+3259                    6.80e+02  1.4e+02       12.0000    -30530  020.9163  +33.2557
   325  WN B0120.8+3259A                   4.27e+02  8.5e+01       12.0000     30530  020.9079  +33.2598
   325  WN B0120.8+3259B                   2.53e+02  5.1e+01       12.0000    -30530  020.9313  +33.2462
  1400  NVSS J012337+331534                6.17e+01  1.2e+01       45.0000     30530  020.9083  +33.2594
  1400  NVSS J012343+331500                3.71e+01  7.4e+00       45.0000    -30530  020.9310  +33.2502
  2380  UGC 938                            3.50e+01  7.0e+00      162.0000     30530  020.9167  +33.2561
  2380  UGC 939                            2.80e+01  5.6e+00      162.0000    -30530  020.9193  +33.2806

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