Complement to VIII/85A

Source PMN_J1814-1732: 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  


 1400  NVSS J181449-173243               8.77e+02  1.8e+02      45.00  107050 0    0.14    2.49  273.7083  -17.5454
 2700  F3R 451                           1.11e+03  2.2e+02     150.00  107050 0    0.14    2.49  273.7121  -17.5503
 4850  PMN J1814-1732                    1.05e+03  2.1e+02     168.00  107050 0    0.14    2.49  273.7163  -17.5450

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  


  1400  GPSR 013.211-0.143                4.74e+02  9.5e+01       5.00  -107050  273.7077  -17.5450
  1400  NVSS J181430-173212               3.10e+00  6.0e-01      45.00  -107050  273.6283  -17.5369
  1400  NVSS J181441-172846               3.80e+00  8.0e-01      45.00  -107050  273.6711  -17.4796
  1400  NVSS J181449-173243               8.77e+02  1.8e+02      45.00   107050  273.7083  -17.5454
  1400  [WBH2005] G13.210-0.143           4.39e+02  8.8e+01       6.00  -107050  273.7083  -17.5458
  2695  RFS 196                           1.11e+03  2.2e+02     294.00  -107050  273.7116  -17.5503
  2700  F3R 451                           1.11e+03  2.2e+02     150.00   107050  273.7121  -17.5503
  2700  [PBD2003] G013.2-00.1             1.30e+03  2.6e+02     480.00  -107050  273.6625  -17.5353
  4850  PMN J1814-1732                    1.05e+03  2.1e+02     168.00   107050  273.7163  -17.5450
  4875  [ADP79] 323                       1.27e+03  2.5e+02     156.00  -107050  273.7071  -17.5481
  4900  GPSR5 013.210-0.144               7.39e+02  1.5e+02       4.02  -107050  273.7081  -17.5461
  5000  [HCS79] B181153.0-173250.7        1.06e+03  2.1e+02      32.40  -107050  273.6991  -17.5312
  8350  GPA1 013.32+0.08                  4.90e+04  9.8e+03     582.00  -107050  273.5567  -17.3453
 14350  GPA 013.32+0.08                   3.74e+04  7.5e+03     396.00  -107050  273.5471  -17.3739

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