Complement to VIII/85A

Source BWE_1148+2242: 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 J1151.0+2226                 6.40e+03  1.3e+03      79.98   49521 4   -1.05    5.78  177.7592  +22.4378
  178  4C +22.31                         2.40e+03  7.2e+02     690.00   49521 4   -1.04    5.75  177.7575  +22.4683
  365  TXS 1148+227                      1.35e+03  2.7e+02       6.00   49521 4   -1.04    5.75  177.7589  +22.4371
  408  B2.4 1148+22                      1.19e+03  2.4e+02       0.00   49521 4   -1.04    5.75  177.7608  +22.4333
 1400  NVSS J115102+222613               2.94e+02  5.9e+01      45.00   49521 4   -1.05    5.76  177.7597  +22.4371
 1400  WB 1148+2242                      3.01e+02  6.0e+01     120.00   49521 4   -1.06    5.80  177.7529  +22.4267
 4850  87GB 114825.7+224219              7.80e+01  1.6e+01     138.00   49521 4   -1.04    5.75  177.7529  +22.4272
 4850  BWE 1148+2242                     7.60e+01  1.5e+01     138.00   49521 4   -1.04    5.75  177.7529  +22.4267
 4850  GB6 B1148+2242                    6.70e+01  1.3e+01     108.00   49521 4   -1.04    5.75  177.7529  +22.4292

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 J1151.0+2226                 6.40e+03  1.3e+03      79.98    49521  177.7592  +22.4378
   178  4C +22.31                         2.40e+03  7.2e+02     690.00    49521  177.7575  +22.4683
   408  B2.4 1148+22                      1.19e+03  2.4e+02       0.00    49521  177.7608  +22.4333
  1400  FIRST J115101.1+222614            8.73e+01  1.8e+01       5.00   -49521  177.7547  +22.4375
  1400  FIRST J115101.8+222615            6.09e+01  1.2e+01       5.00   -49521  177.7576  +22.4375
  1400  FIRST J115103.2+222612            1.34e+02  2.7e+01       5.00   -49521  177.7636  +22.4368
  4850  87GB 114825.7+224219              7.80e+01  1.6e+01     138.00    49521  177.7529  +22.4272

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