Complement to VIII/104

Source PMN_J0134-3629: 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 J110921.0+213802              9.45e+01  1.9e+01       25.0020  144288   -0.15     2.30  167.3375  +21.6340
  200  GLEAM J110921+213805                  1.17e+02  3.0e+01      120.0000  144288   -0.15     2.30  167.3378  +21.6349
 1400  FIRST14 J110920.9+213801              6.76e+01  1.4e+01        4.9998  144288   -0.13     2.27  167.3372  +21.6338
 1400  NVSS J110920+213803                   5.85e+01  1.2e+01       45.0000  144288   -0.13     2.27  167.3374  +21.6342
 4850  87GB 110640.0+215402                  5.92e+01  1.2e+01      138.0000  144288   -0.15     2.30  167.3325  +21.6294
 4850  GB6 B1106+2154                        3.39e+01  6.8e+00      108.0000  144288   -0.35     2.88  167.3313  +21.6322

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  


   145  [JAP2011] J23.55-36.52             2.61e+04  5.2e+03     1560.0000   -144288  023.5500  -36.5200
   150  TGSSADR J013412.0-362915           1.29e+04  2.6e+03       25.0020   -144288  023.5504  -36.4875
   182  KGS J013412-362909                 7.10e+03  1.4e+03        2.4000   -144288  023.5511  -36.4861
   200  GLEAM J013411-362913               1.52e+04  3.0e+03      120.0000   -144288  023.5486  -36.4872
   408  MRC 0131-367A                      4.90e+03  9.8e+02      120.0000   -144288  023.5508  -36.4872
   843  MOST 0131-367                      1.03e+04  2.1e+03       43.9800   -144288  023.4854  -36.4856
   843  SUMSS J013413-362857               4.81e+03  9.6e+02       18.0000   -144288  023.5542  -36.4827
  1400  NVSS J013414-362833                1.81e+03  3.6e+02       45.0000   -144288  023.5595  -36.4759
  2307  SPASS J013356-362905               5.85e+03  1.2e+03      645.0000   -144288  023.4862  -36.4848
  4850  PMN J0134-3629                     1.51e+03  3.0e+02      168.0000   -144288  023.5500  -36.4872

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