Complement to VIII/104

Source MRC_1156-094: 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 J115912.5-094053                2.59e+03  5.2e+02       75.0000  163294   -0.37     4.14  179.8021  -09.6816
  150  TGSSADR J115912.6-094052              2.18e+03  4.4e+02       25.0020  163294   -0.36     4.08  179.8027  -09.6814
  200  GLEAM J115912-094054                  1.80e+03  3.6e+02      120.0000  163294   -0.37     4.14  179.8035  -09.6817
  365  TXS 1156-094                          1.77e+03  3.5e+02        6.0000  163294   -0.37     4.14  179.8030  -09.6810
  408  MRC 1156-094                          1.56e+03  3.1e+02      120.0000  163294   -0.37     4.14  179.8038  -09.6817
 1400  NVSS J115912-094051                   1.03e+03  2.1e+02       45.0000  163294   -0.37     4.14  179.8029  -09.6810
 2307  SPASS J115911-094112                  7.09e+02  1.4e+02      645.0000  163294   -0.38     4.16  179.7993  -09.6868
 2700  PKS J1159-0941                        7.50e+02  1.5e+02       60.0000  163294   -0.37     4.14  179.8029  -09.6811
 4850  PMN J1159-0941                        5.84e+02  1.2e+02      168.0000  163294   -0.38     4.16  179.8025  -09.6853
 8400  CRATES J115912-094107                 4.29e+02  8.6e+01        6.0000  163294   -0.34     4.06  179.8021  -09.6794
 8400  PKS8400 J1159-0940                    3.90e+02  7.8e+01      162.0000  163294   -0.37     4.14  179.8030  -09.6811
22000  K-RFC J1159-0940                      4.80e+02  9.6e+01      126.0000  163294   -0.37     4.14  179.8035  -09.6811

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 J025343.9-474926           1.01e+02  2.0e+01       25.0020   -163294  043.4333  -47.8240
   200  GLEAM J025345-474916               1.60e+02  3.2e+01      120.0000   -163294  043.4400  -47.8213
   843  SUMSS J025344-474922               3.24e+01  6.5e+00       18.0000   -163294  043.4372  -47.8230

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