Complement to VIII/104

Source NVSS_J114048-262909: 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 J114048.3-262905                2.67e+04  5.3e+03       75.0000  163175   -1.22     6.76  175.2017  -26.4849
   80  Cula 1138-262                         2.70e+04  5.4e+03      222.0000  163175   -1.22     6.76  175.2095  -26.4936
  150  TGSSADR J114048.3-262911              1.25e+04  2.5e+03       25.0020  163175   -1.22     6.76  175.2015  -26.4864
  160  Culb 1138-262                         1.20e+04  2.4e+03      111.0000  163175   -1.22     6.76  175.2095  -26.4936
  200  GLEAM J114048-262908                  8.19e+03  1.6e+03      120.0000  163175   -1.22     6.76  175.2018  -26.4856
  365  TXS 1138-262                          4.53e+03  9.1e+02        6.0000  163175   -1.22     6.76  175.2015  -26.4863
  408  MRC 1138-262                          4.12e+03  8.2e+02      120.0000  163175   -1.22     6.76  175.2017  -26.4858
 1400  NVSS J114048-262909                   8.70e+02  1.7e+02       45.0000  163175   -1.22     6.76  175.2017  -26.4859
 1465  [RLM94] 1138-262A                     7.28e+02  1.5e+02        4.5000  163175   -1.22     6.76  175.2038  -26.4858
 2307  SPASS J114041-262959                  4.44e+02  8.9e+01      645.0000  163175   -1.22     6.76  175.1738  -26.4997
 2700  PKS J1140-2628                        3.80e+02  7.6e+01       60.0000  163175   -1.19     6.66  175.1904  -26.4825
 4850  PMN J1140-2629                        1.42e+02  2.8e+01      168.0000  163175   -1.22     6.76  175.1912  -26.4847

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 J024021.2-495532           4.68e+01  9.4e+00       25.0020   -163175  040.0887  -49.9258
   200  GLEAM J024021-495520               6.91e+01  1.4e+01      120.0000   -163175  040.0883  -49.9224
   843  SUMSS J024021-495530               2.20e+01  4.4e+00       18.0000   -163175  040.0889  -49.9251

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