Complement to VIII/104

Source UGC_7494: 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  


   74  VLSSr J122505.0+125318                1.55e+04  3.1e+03       75.0000  162071   -0.34     4.90  186.2710  +12.8885
  150  TGSSADR J122504.2+125309              1.53e+04  3.1e+03       25.0020  162071   -0.55     5.46  186.2679  +12.8858
  200  GLEAM J122504+125308                  1.57e+04  3.1e+03      120.0000  162071   -0.50     5.35  186.2702  +12.8857
  408  MRC 1222+131                          1.22e+04  2.4e+03      120.0000  162071   -0.51     5.36  186.2713  +12.8869
 1400  WB 1222+1309                          6.50e+03  1.3e+03      120.0000  162071   -0.46     5.27  186.2708  +12.8894
 2380  UGC 7494                              3.64e+03  7.3e+02      162.0000  162071   -0.51     5.36  186.2654  +12.8870
 2700  PKS J1225+1253                        4.20e+03  8.4e+02       60.0000  162071   -0.51     5.37  186.2679  +12.8836
 4850  87GB 122232.6+131000                  4.00e+03  8.0e+02      138.0000  162071   -0.39     5.02  186.2700  +12.8897
 4850  BWE 1222+1309                         3.58e+03  7.2e+02      138.0000  162071   -0.51     5.37  186.2708  +12.8894
 4850  GB6 B1222+1309                        3.58e+03  7.2e+02      108.0000  162071   -0.38     5.01  186.2692  +12.8886
 4850  IRAS F12225+1309                      2.86e+03  5.7e+02      210.0000  162071   -0.50     5.35  186.2620  +12.8869
 4850  MITG J122505+1252                     2.74e+03  5.5e+02      258.0000  162071   -0.53     5.46  186.2721  +12.8719

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 J012056.2+003902           2.91e+01  6.5e+00       25.0020   -162071  020.2345  +00.6506
   200  GLEAM J012054+003848               1.04e+02  2.5e+01      120.0000   -162071  020.2262  +00.6468
  1400  [HBW2011] J012056.2+003903         3.10e+00  6.0e-01        1.8000   -162071  020.2342  +00.6509

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