Complement to VIII/104

Source BWE_1228+1240: 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 J123049.6+122321              4.80e+05  9.6e+04       25.0020  162257   -0.66     7.21  187.7068  +12.3894
  160  Culb 1228+126                         5.66e+05  1.1e+05      111.0000  162257   -0.65     7.18  187.7058  +12.3869
 1400  FIRST14 J123049.3+122323              1.22e+05  2.4e+04        4.9998  162257   -0.68     7.25  187.7055  +12.3899
 1400  NVSS J123049+122321                   1.38e+05  2.8e+04       45.0000  162257   -0.65     7.18  187.7061  +12.3893
 2380  UGC 7654                              1.34e+05  2.7e+04      162.0000  162257   -0.66     7.21  187.7058  +12.3911
 2700  PKS J1230+1223                        1.20e+05  2.4e+04       60.0000  162257   -0.65     7.18  187.7058  +12.3911
 4850  87GB 122819.0+124029                  6.12e+04  1.2e+04      138.0000  162257   -0.66     7.21  187.7121  +12.3986
 4850  BWE 1228+1240                         5.97e+04  1.2e+04      138.0000  162257   -0.66     7.21  187.7100  +12.3978
 4850  GB6 B1228+1240                        7.20e+04  1.4e+04      108.0000  162257   -0.65     7.18  187.7033  +12.3933
 4850  IRAS F12282+1240                      7.00e+04  1.4e+04      210.0000  162257   -0.65     7.18  187.7012  +12.3931
 4885  RGB 1230+123                          5.90e+04  1.2e+04        4.0200  162257   -0.66     7.21  187.7059  +12.3911
22000  K-RFC J1230+1223                      2.01e+04  4.0e+03      126.0000  162257   -0.65     7.18  187.7055  +12.3911

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  [TRC2006]b J0216.6-0024            3.00e-01  1.0e-01       30.0000   -162257  034.1534  -00.4150
   200  GLEAM J021637-002454               1.72e+02  3.4e+01      120.0000   -162257  034.1544  -00.4153
  1400  [HBW2011] J021636.1-002445         4.40e+00  9.0e-01        1.8000   -162257  034.1504  -00.4126

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