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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
38 8C 225012+642414 2.82e+04 5.6e+03 270.00 93335 0 -0.79 5.80 343.0167 +64.6697 74 VLSS J2252.1+6440 2.16e+04 4.3e+03 79.98 93335 0 -0.79 5.80 343.0250 +64.6697 178 4C +64.24 1.03e+04 3.1e+03 690.00 93335 0 -0.79 5.80 343.0138 +64.6783 232 MY 225012.2+644037.4 1.00e+04 2.0e+03 150.00 93335 0 -0.79 5.80 343.0183 +64.6771 325 WN B2250.2+6424 8.34e+03 1.7e+03 12.00 93335 0 -0.79 5.80 343.0191 +64.6709 365 TXS 2250+644 6.10e+03 1.2e+03 6.00 93335 0 -0.79 5.80 343.0234 +64.6700 1400 NVSS J225205+644010 2.29e+03 4.6e+02 45.00 93335 0 -0.79 5.80 343.0239 +64.6695 1400 WB 2250+6424 2.36e+03 4.7e+02 120.00 93335 0 -0.79 5.80 343.0213 +64.6667 1410 RRF 1069 2.21e+03 4.4e+02 564.00 93335 0 -0.79 5.80 343.0412 +64.6736 2700 F3R 3408 1.28e+03 2.6e+02 150.00 93335 0 -0.79 5.80 343.0333 +64.6675 4850 87GB 225012.7+642402 7.76e+02 1.6e+02 138.00 93335 0 -0.79 5.80 343.0208 +64.6664 4850 BWE 2250+6424 6.91e+02 1.4e+02 138.00 93335 0 -0.79 5.80 343.0213 +64.6667 4850 GB6 B2250+6424 7.01e+02 1.4e+02 108.00 93335 0 -0.79 5.80 343.0213 +64.6686
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%