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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) |
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] Source parameters based on positional cross-id[spectrum] (1497216 rows) |
nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
74 VLSS J1242.1+3232 2.20e+03 4.4e+02 79.98 -189377 190.5304 +32.5417 151 7C 123922.69+324731.00 3.58e+03 7.5e+02 70.20 -189377 190.4538 +32.5178 151 7C 123941.60+324854.00 3.80e+03 7.6e+02 70.20 -189377 190.5321 +32.5411 232 MY 123939.1+323241.4 2.09e+03 4.2e+02 150.00 -189377 190.5221 +32.5448 325 WN B1239.6+3248 2.91e+03 5.8e+02 12.00 -189377 190.5216 +32.5402 325 WN B1239.6+3248B 8.56e+02 1.7e+02 12.00 -189377 190.5273 +32.5399 325 WN B1239.6+3248C 1.54e+03 3.1e+02 12.00 -189377 190.5430 +32.5436 408 B2.1 1239+32 3.80e+03 7.6e+02 0.00 -189377 190.5213 +32.5417 1400 FIRST J124205.1+323223 5.68e+01 1.1e+01 5.00 -189377 190.5214 +32.5397 2380 UGC 7865 3.40e+02 6.8e+01 162.00 -189377 190.5325 +32.5408 4850 87GB 123941.4+324853 4.25e+02 8.5e+01 138.00 -189377 190.5317 +32.5408 4850 GB6 B1239+3248 4.63e+02 9.3e+01 108.00 -189377 190.5292 +32.5381 4850 IRAS F12396+3249 4.20e+02 8.4e+01 210.00 -189377 190.5275 +32.5433 4850 MITG J124203+3232 2.99e+02 6.0e+01 258.00 -189377 190.5146 +32.5389 10550 [NKB95] N4631 2.65e+02 5.3e+01 69.00 -189377 190.5317 +32.5411
Note: For the spectrum finding algorithm, the errors have been increased by 50%