Complement to VIII/85A

Source [PBD2003]_G015.1-00.7: 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  


 2695  RFS 215                           4.80e+05  9.6e+04     294.00   77567 0    0.18    5.06  275.1304  -16.1861
 2700  F3R 502                           4.80e+05  9.6e+04     150.00   77567 0    0.19    5.01  275.1304  -16.1861
 2700  [PBD2003] G015.1-00.7             5.52e+05  1.1e+05     480.00   77567 0    0.19    5.01  275.1562  -16.1475
 8350  GPA1 015.10-0.68                  6.47e+05  1.3e+05     582.00   77567 0    0.11    5.36  275.1392  -16.1325

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  


   365  TXS 1817-161                      1.22e+03  2.4e+02       6.00   -77567  275.0997  -16.1301
  1400  [WBH2005] G15.036-0.678           1.59e+03  3.2e+02       6.00   -77567  275.1048  -16.1921
  1400  [WBH2005] G15.038-0.674           9.54e+02  1.9e+02       6.00   -77567  275.1022  -16.1886
  1410  RRF 95                            5.27e+05  1.1e+05     564.00   -77567  275.1292  -16.1889
  2695  RFS 215                           4.80e+05  9.6e+04     294.00    77567  275.1304  -16.1861
  2700  F3R 502                           4.80e+05  9.6e+04     150.00    77567  275.1304  -16.1861
  2700  [PBD2003] G015.0-00.7             4.89e+05  9.8e+04     480.00   -77567  275.1071  -16.2356
  2700  [PBD2003] G015.1-00.7             5.52e+05  1.1e+05     480.00    77567  275.1562  -16.1475
  4850  PMN J1820-1609                    6.13e+04  1.2e+04     168.00   -77567  275.0733  -16.1564
  4875  [ADP79] 369                       4.49e+04  9.0e+03     156.00   -77567  275.1113  -16.2000
  8350  GPA1 015.10-0.68                  6.47e+05  1.3e+05     582.00    77567  275.1392  -16.1325
 14350  GPA 015.05-0.66                   9.70e+03  1.9e+03     396.00   -77567  275.0962  -16.1669
 14350  GPA 015.10-0.68                   6.64e+05  1.3e+05     396.00   -77567  275.1429  -16.1361

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