Complement to VIII/104

Source GB6_B1232+3637: 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 J123505.8+362118              1.12e+02  2.2e+01       25.0020  162410    0.17     1.69  188.7742  +36.3552
  325  WN B1232.6+3637                       1.00e+02  2.0e+01       12.0000  162410    0.17     1.69  188.7727  +36.3559
 1400  FIRST14 J123505.7+362119              1.75e+02  3.5e+01        4.9998  162410    0.17     1.69  188.7741  +36.3553
 1400  NVSS J123505+362120                   1.54e+02  3.1e+01       45.0000  162410    0.17     1.69  188.7742  +36.3556
 4850  87GB 123239.4+363756                  2.50e+02  5.0e+01      138.0000  162410    0.17     1.69  188.7746  +36.3569
 4850  BWE 1232+3637                         2.51e+02  5.0e+01      138.0000  162410    0.17     1.69  188.7742  +36.3572
 4850  GB6 B1232+3637                        2.34e+02  4.7e+01      108.0000  162410    0.17     1.69  188.7742  +36.3556
 4850  MITG J123503+3621                     2.49e+02  5.0e+01      258.0000  162410    0.17     1.69  188.7658  +36.3558
 5000  VIPS J12350+3621                      2.02e+02  4.0e+01        0.0009  162410    0.15     1.72  188.7742  +36.3554
 8400  CLASS J123505.8079+362119.303         2.06e+02  4.1e+01        0.3300  162410    0.17     1.69  188.7742  +36.3554
 8400  CRATES J123505+362120                 2.06e+02  4.1e+01        6.0000  162410    0.17     1.69  188.7742  +36.3554
 8400  JVAS J1235+363                        2.00e+02  4.0e+01        0.3300  162410    0.17     1.69  188.7742  +36.3554

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 J014706.6-011543           5.33e+01  1.1e+01       25.0020   -162410  026.7776  -01.2620
   200  GLEAM J014707-011542               8.08e+01  1.6e+01      120.0000   -162410  026.7823  -01.2617
  1400  [HBW2011] J014706.7-011543         2.40e+00  5.0e-01        1.8000   -162410  026.7783  -01.2620

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