Complement to VIII/104

Source CRATES_J103906-154103: 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 J103906.7-154107              3.45e+02  6.9e+01       25.0020  145542    0.02     2.58  159.7780  -15.6853
  200  GLEAM J103906-154102                  3.45e+02  6.9e+01      120.0000  145542    0.02     2.58  159.7768  -15.6841
  325  WISH B1036.6-1525                     4.72e+02  9.4e+01       18.0000  145542    0.02     2.58  159.7776  -15.6847
  365  TXS 1036-154                          4.30e+02  8.6e+01        6.0000  145542    0.02     2.58  159.7776  -15.6855
 1400  NVSS J103906-154107                   4.50e+02  9.0e+01       45.0000  145542    0.02     2.58  159.7781  -15.6854
 1465  [P82] 1036-154                        5.40e+02  1.1e+02       25.8000  145542    0.02     2.58  159.7778  -15.6852
 2307  SPASS J103904-154112                  3.46e+02  6.9e+01      645.0000  145542    0.02     2.58  159.7693  -15.6868
 4850  PMN J1039-1541                        6.26e+02  1.3e+02      168.0000  145542    0.02     2.58  159.7775  -15.6842
 4885  [P82a] 1036-154                       3.80e+02  7.6e+01        6.0000  145542    0.02     2.58  159.7778  -15.6852
 8400  CRATES J103906-154103                 3.92e+02  7.8e+01        6.0000  145542    0.02     2.58  159.7780  -15.6852
 8400  PKS8400 J1039-1541                    6.70e+02  1.3e+02      162.0000  145542    0.06     2.43  159.7780  -15.6852
22000  K-RFC J1039-1541                      4.70e+02  9.4e+01      126.0000  145542    0.02     2.58  159.7785  -15.6852

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 J015604.3-053924           3.65e+01  7.3e+00       25.0020   -145542  029.0182  -05.6569
   200  GLEAM J015602-053923               9.42e+01  1.9e+01      120.0000   -145542  029.0106  -05.6566
  1400  NVSS J015603-053924                1.13e+01  2.3e+00       45.0000   -145542  029.0138  -05.6567

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