| Postscript Figure | Additional frequencies and fluxes in ν and S | Data as a Table |
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"-c="
| 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] The parameters of the radio spectra[image][spectrum] (631736 rows) |
nu Name S(nu) e beam Seq n a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
365 TXS 0544+273 3.88e+02 7.8e+01 6.00 23100 0 0.00 2.45 086.8927 +27.3661 408 B2.2 0544+27 2.62e+02 5.2e+01 0.00 23100 0 0.21 1.94 086.8971 +27.3417 1400 NVSS J054734+272157 3.37e+02 6.7e+01 45.00 23100 0 0.21 1.94 086.8923 +27.3658 1400 WB 0544+2720 3.56e+02 7.1e+01 120.00 23100 0 0.24 1.83 086.8929 +27.3622 1410 RRF 1945 3.85e+02 7.7e+01 564.00 23100 0 0.21 1.94 086.8983 +27.3514 2700 F3R 5081 4.40e+02 8.8e+01 150.00 23100 0 0.21 1.94 086.8946 +27.3625 4850 87GB 054426.0+272041 5.20e+02 1.0e+02 138.00 23100 0 0.06 2.43 086.8925 +27.3617 4850 BWE 0544+2720 5.18e+02 1.0e+02 138.00 23100 0 0.06 2.43 086.8929 +27.3622 4850 GB6 B0544+2720 5.25e+02 1.0e+02 108.00 23100 0 0.00 2.45 086.8917 +27.3636 4850 MITG J054734+2722 6.36e+02 1.3e+02 258.00 23100 0 0.06 2.43 086.8937 +27.3714 8400 CLASS J054734.1484+272156.841 2.74e+02 5.5e+01 0.33 23100 0 0.01 2.43 086.8923 +27.3658 8400 JVAS J0547+2721 2.69e+02 5.4e+01 0.33 23100 0 0.00 2.45 086.8923 +27.3658
| VIII/85A/waste Post annotation | SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp] Source parameters based on positional cross-id[spectrum] (1497216 rows) |
Note: For the spectrum finding algorithm, the errors have been increased by 50%