Complement to VIII/104

Source K-RFC_J1141+6410: 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  


  325  WN B1138.4+6426                       1.22e+02  2.4e+01       12.0000  160332    0.22     1.52  175.3012  +64.1684
 1400  FIRST14 J114112.2+641005              2.19e+02  4.4e+01        4.9998  160332    0.23     1.51  175.3010  +64.1681
 1400  NVSS J114112+641005                   2.52e+02  5.0e+01       45.0000  160332    0.00     2.40  175.3009  +64.1682
 1400  WB 1138+6426                          2.75e+02  5.5e+01      120.0000  160332   -0.03     2.55  175.3046  +64.1692
 4850  87GB 113827.0+642646                  3.71e+02  7.4e+01      138.0000  160332    0.22     1.52  175.3042  +64.1689
 4850  BWE 1138+6426                         3.29e+02  6.6e+01      138.0000  160332    0.08     2.09  175.3046  +64.1692
 4850  GB6 B1138+6426                        3.07e+02  6.1e+01      108.0000  160332    0.22     1.52  175.2983  +64.1669
 5000  VIPS J11412+6410                      1.64e+02  3.3e+01        0.0009  160332    0.31     1.14  175.3009  +64.1682
 8400  CLASS J114112.2294+641005.483         2.55e+02  5.1e+01        0.3300  160332    0.31     1.14  175.3009  +64.1682
 8400  CRATES J114111+641001                 2.55e+02  5.1e+01        6.0000  160332    0.22     1.52  175.3010  +64.1682
 8400  JVAS J1141+641                        2.53e+02  5.1e+01        0.3300  160332    0.22     1.52  175.3009  +64.1682
22000  K-RFC J1141+6410                      2.50e+02  5.0e+01      126.0000  160332    0.22     1.52  175.3005  +64.1682

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 J013344.0-050353           8.35e+01  1.7e+01       25.0020   -160332  023.4337  -05.0648
   200  GLEAM J013344-050349               1.20e+02  2.4e+01      120.0000   -160332  023.4343  -05.0639
  1400  FIRST14 J013344.1-050347           6.10e+00  1.2e+00        4.9998   -160332  023.4341  -05.0633

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