Complement to VIII/104

Source BWE_1227+0816: 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 J122946.6+080006              1.14e+03  2.3e+02       25.0020  162238   -0.76     4.75  187.4446  +08.0018
  200  GLEAM J122946+075958                  1.26e+03  2.5e+02      120.0000  162238   -0.75     4.71  187.4447  +07.9995
 1400  NVSS J122946+080002                   2.20e+02  4.4e+01       45.0000  162238   -0.74     4.67  187.4442  +08.0008
 2380  UGC 7629                              1.32e+02  2.6e+01      162.0000  162238   -0.74     4.67  187.4450  +08.0000
 2700  RGB11 J1229.8+0800                    1.54e+02  3.1e+01      258.0000  162238   -0.74     4.67  187.4458  +08.0044
 4850  87GB 122714.6+081649                  1.11e+02  2.2e+01      138.0000  162238   -0.74     4.66  187.4467  +08.0042
 4850  BWE 1227+0816                         1.09e+02  2.2e+01      138.0000  162238   -0.75     4.71  187.4471  +08.0047
 4850  GB6 B1227+0816                        8.60e+01  1.7e+01      108.0000  162238   -0.75     4.71  187.4471  +08.0017
 4850  MITG J122942+0800                     8.50e+01  1.7e+01      258.0000  162238   -0.74     4.67  187.4283  +08.0086
 4885  RGB 1229+080                          8.60e+01  1.7e+01        4.0200  162238   -0.74     4.67  187.4449  +08.0004
 5000  RGB6 J1229.8+0800                     9.30e+01  1.9e+01      144.0000  162238   -0.75     4.71  187.4458  +08.0044
10700  RGB2 J1229.8+0800                     4.80e+01  9.6e+00       72.0000  162238   -0.75     4.70  187.4458  +08.0044

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 J013603.2-001720           3.49e+01  7.0e+00       25.0020   -162238  024.0134  -00.2891
   200  GLEAM J013603-001732               5.58e+01  1.4e+01      120.0000   -162238  024.0156  -00.2924
  1400  [HBW2011] J013603.1-001722         5.10e+00  1.0e+00        1.8000   -162238  024.0132  -00.2896

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