Complement to VIII/85A

Source 7C_125834.39+383042.00: 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 2 columns 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/85A/spectra
Post annotation 		SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
2010A&A...511A..53V

The parameters of the radio spectra[image][spectrum] (631736 rows)		img(gal)
start AladinLite 
  nu   Name                               S(nu)       e        beam      Seq  n     a       b     RAJ2000   DEJ2000
 MHz                                       mJy       mJy      arcsec                      [mJy]     deg       deg  


   74  VLSS J1300.9+3814                 1.46e+03  2.9e+02      79.98   61565 0   -1.01    5.05  195.2267  +38.2431
  151  6C 125833+383120                  5.70e+02  1.1e+02     252.00   61565 0   -1.01    5.06  195.2237  +38.2533
  151  7C 125834.39+383042.00            6.42e+02  1.3e+02      70.20   61565 0   -1.01    5.05  195.2271  +38.2428
  325  WN B1258.5+3830                   3.24e+02  6.5e+01      12.00   61565 0   -1.02    5.07  195.2272  +38.2443
  408  5C12a 517                         2.50e+02  1.0e+02      79.98   61565 0   -1.01    5.05  195.2266  +38.2418
  408  B2.3 1258+38                      3.05e+02  6.1e+01       0.00   61565 0   -1.01    5.06  195.2279  +38.2467
  408  B3 1258+385                       2.30e+02  4.6e+01      84.00   61565 0   -1.01    5.05  195.2283  +38.2444
 1400  FIRST J130054.6+381440            7.24e+01  1.4e+01       5.00   61565 0   -1.02    5.07  195.2276  +38.2446
 1400  NVSS J130054+381439               7.39e+01  1.5e+01      45.00   61565 0   -1.01    5.05  195.2277  +38.2443

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/85A/waste
Post annotation 		SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
2010A&A...511A..53V

Source parameters based on positional cross-id[spectrum] (1497216 rows)		img(gal)
start AladinLite 
  nu    Name                               S(nu)       e        beam      Seq     RAJ2000   DEJ2000
  MHz                                       mJy       mJy      arcsec               deg       deg  


    74  VLSS J1300.9+3814                 1.46e+03  2.9e+02      79.98    61565  195.2267  +38.2431
   151  6C 125833+383120                  5.70e+02  1.1e+02     252.00    61565  195.2237  +38.2533
   232  MY 125830.6+381334.7              1.70e+02  5.7e+01     150.00   -61565  195.2113  +38.2263
   365  TXS 1258+385                      6.34e+02  1.3e+02       6.00   -61565  195.2321  +38.2456
   408  5C12a 517                         2.50e+02  1.0e+02      79.98    61565  195.2266  +38.2418
   408  B2.3 1258+38                      3.05e+02  6.1e+01       0.00    61565  195.2279  +38.2467
  1400  NVSS J130054+381439               7.39e+01  1.5e+01      45.00    61565  195.2277  +38.2443

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