| Postscript Figure | Additional frequencies and fluxes in ν and S | Data as a Table |
| ||||||
"-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
325 WN B0504.0+3834 4.91e+02 9.8e+01 12.00 18438 0 -0.48 3.98 076.8713 +38.6450 365 TXS 0504+385 6.08e+02 1.2e+02 6.00 18438 0 -0.48 3.98 076.8718 +38.6450 408 B2.3 0504+38 6.52e+02 1.3e+02 0.00 18438 0 -0.60 4.36 076.8738 +38.6483 408 B3 0504+385 5.30e+02 1.1e+02 84.00 18438 0 -0.48 3.98 076.8692 +38.6467 1400 NVSS J050729+383842 3.77e+02 7.5e+01 45.00 18438 0 -0.50 4.05 076.8716 +38.6452 1400 WB 0504+3834 2.90e+02 5.8e+01 120.00 18438 0 -0.55 4.19 076.8692 +38.6456 1410 RRF 1793 2.30e+02 4.6e+01 564.00 18438 0 -0.48 3.98 076.8583 +38.6400 2700 F3R 4767 2.70e+02 5.4e+01 150.00 18438 0 -0.57 4.29 076.8787 +38.6356 4850 87GB 050403.1+383450 1.57e+02 3.1e+01 138.00 18438 0 -0.58 4.32 076.8696 +38.6458 4850 BWE 0504+3834 1.39e+02 2.8e+01 138.00 18438 0 -0.59 4.32 076.8692 +38.6456 4850 GB6 B0504+3834 1.61e+02 3.2e+01 108.00 18438 0 -0.57 4.29 076.8696 +38.6439 4850 MITG J050725+3838 1.37e+02 2.7e+01 258.00 18438 0 -0.60 4.36 076.8554 +38.6486
| 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%