Complement to VIII/85A

Source PMN_J1822-0939: 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  


  365  TXS 1819-096                      1.11e+04  2.2e+03       6.00  107051 4   -0.58    5.52  275.6199  -09.6492
 1400  NVSS J182228-093857               5.84e+03  1.2e+03      45.00  107051 4   -0.58    5.52  275.6196  -09.6492
 2700  F3R 704                           3.51e+03  7.0e+02     150.00  107051 4   -0.58    5.52  275.6233  -09.6478
 4850  PMN J1822-0939                    2.44e+03  4.9e+02     168.00  107051 4   -0.59    5.54  275.6183  -09.6528

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 J1822.4-0938                 8.87e+03  1.8e+03      79.98  -107051  275.6208  -09.6489
    80  Cula 1819-096                     1.20e+04  2.4e+03     222.00  -107051  275.6208  -09.6511
   160  Culb 1819-096                     1.24e+04  2.5e+03     111.00  -107051  275.6208  -09.6511
   365  TXS 1819-096                      1.11e+04  2.2e+03       6.00   107051  275.6199  -09.6492
  1400  NVSS J182228-093857               5.84e+03  1.2e+03      45.00   107051  275.6196  -09.6492
  1400  NVSS J182228-094244               1.48e+01  3.0e+00      45.00  -107051  275.6186  -09.7123
  1400  NVSS J182234-094305               7.10e+00  1.6e+00      45.00  -107051  275.6430  -09.7181
  1400  NVSS J182240-093803               9.30e+00  1.9e+00      45.00  -107051  275.6695  -09.6342
  1410  RRF 136                           5.97e+03  1.2e+03     564.00  -107051  275.6154  -09.6686
  2700  F3R 704                           3.51e+03  7.0e+02     150.00   107051  275.6233  -09.6478
  2700  [PBD2003] G021.0+02.0             3.80e+03  1.7e+03     480.00  -107051  275.5579  -09.6717
  4850  PMN J1822-0939                    2.44e+03  4.9e+02     168.00   107051  275.6183  -09.6528
  5000  [HCS79] B181946.5-093939.0        1.85e+03  3.7e+02      32.40  -107051  275.6313  -09.6352

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