Complement to VIII/85A

Source BWE_0734+5420: 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  


  151  6C 073440+542020                  6.20e+02  1.2e+02     252.00   31553 1   -0.83    4.60  114.6608  +54.2250
  151  7C 073440.10+542018.00            6.74e+02  1.3e+02      70.20   31553 1   -0.79    4.52  114.6608  +54.2244
  232  MY 073441.8+541306.2              3.70e+02  7.4e+01     150.00   31553 1   -0.73    4.32  114.6679  +54.2184
  325  WN B0734.6+5420                   3.94e+02  7.9e+01      12.00   31553 1   -0.83    4.64  114.6606  +54.2236
  365  TXS 0734+543                      3.61e+02  7.2e+01       6.00   31553 1   -0.73    4.31  114.6604  +54.2236
 1400  FIRST J073838.4+541326            9.76e+01  2.0e+01       5.00   31553 1   -0.87    4.72  114.6601  +54.2240
 1400  NVSS J073838+541325               1.06e+02  2.1e+01      45.00   31553 1   -0.83    4.64  114.6604  +54.2239
 4850  87GB 073438.9+542013              4.34e+01  8.7e+00     138.00   31553 1   -0.83    4.60  114.6558  +54.2231
 4850  BWE 0734+5420                     4.20e+01  8.4e+00     138.00   31553 1   -0.79    4.52  114.6550  +54.2233
 4850  GB6 B0734+5420                    3.30e+01  6.6e+00     108.00   31553 1   -0.84    4.63  114.6587  +54.2222
 4885  RGB 0738+542                      3.30e+01  6.6e+00       4.02   31553 1   -0.73    4.32  114.6600  +54.2245

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  


   151  6C 073440+542020                  6.20e+02  1.2e+02     252.00    31553  114.6608  +54.2250
  1400  FIRST J073829.6+541311            4.40e+00  9.0e-01       5.00   -31553  114.6236  +54.2198
  1400  FIRST J073844.0+541139            1.80e+00  4.0e-01       5.00   -31553  114.6834  +54.1942
  1400  NVSS J073829+541306               3.50e+00  7.0e-01      45.00   -31553  114.6227  +54.2183
  4850  87GB 073438.9+542013              4.34e+01  8.7e+00     138.00    31553  114.6558  +54.2231

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