| 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
74 VLSS J0547.7+3137 2.15e+03 4.3e+02 79.98 23106 4 -0.80 4.82 086.9433 +31.6250 232 MY 054430.9+313712.5 5.60e+02 1.1e+02 150.00 23106 4 -0.72 4.56 086.9404 +31.6201 325 WN B0544.5+3136 7.61e+02 1.5e+02 12.00 23106 4 -0.80 4.83 086.9429 +31.6249 365 TXS 0544+316 7.48e+02 1.5e+02 6.00 23106 4 -0.80 4.83 086.9442 +31.6249 408 B2.1 0544+31 6.20e+02 1.2e+02 0.00 23106 4 -0.80 4.83 086.9458 +31.6250 1400 NVSS J054746+313729 1.87e+02 3.7e+01 45.00 23106 4 -0.80 4.83 086.9437 +31.6249 1400 WB 0544+3136 1.99e+02 4.0e+01 120.00 23106 4 -0.80 4.82 086.9471 +31.6233 1410 RRF 1900 2.05e+02 4.1e+01 564.00 23106 4 -0.80 4.83 086.9058 +31.6244 2700 F3R 4991 1.00e+02 2.7e+01 150.00 23106 4 -0.80 4.82 086.9346 +31.6267 4850 87GB 054431.7+313623 8.21e+01 1.6e+01 138.00 23106 4 -0.80 4.83 086.9437 +31.6231 4850 BWE 0544+3136 5.60e+01 1.1e+01 138.00 23106 4 -0.97 5.31 086.9471 +31.6233 4850 GB6 B0544+3136 7.21e+01 1.4e+01 108.00 23106 4 -0.81 4.85 086.9458 +31.6275
| 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%