Complement to VIII/85A

Source PKS_J1347-2422: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
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VIII/85A/spectra
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SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
The parameters of the radio spectra[image][spectrum] (631736 rows)
img(gal)
start AladinLite
No object foundThe 1 column 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/waste
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SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
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
325 WISH B1344.5-2412 1.66e+03 3.3e+02 18.00 -197000 206.8443 -24.4590 325 WISH B1344.5-2412A 4.60e+01 9.2e+00 18.00 -197000 206.8188 -24.3262 325 WISH B1344.5-2412B 4.80e+01 9.6e+00 18.00 -197000 206.8461 -24.3612 408 MRC 1344-241 1.02e+03 2.0e+02 120.00 -197000 206.8071 -24.3819 1400 NVSS J134702-242243 5.40e+00 1.1e+00 45.00 -197000 206.7623 -24.3788 1400 NVSS J134709-242242 2.91e+02 5.8e+01 45.00 -197000 206.7886 -24.3784 1400 NVSS J134710-242406 3.70e+00 7.0e-01 45.00 -197000 206.7954 -24.4017 1400 NVSS J134718-242205 2.24e+02 4.5e+01 45.00 -197000 206.8261 -24.3681 1400 NVSS J134723-242216 6.66e+01 1.3e+01 45.00 -197000 206.8474 -24.3711 2700 PKS J1347-2422 3.90e+02 7.8e+01 60.00 -197000 206.8058 -24.3736 4850 PMN J1347-2422 1.87e+02 3.7e+01 168.00 -197000 206.8054 -24.3806

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