Complement to VIII/85A

Source DRAOP_12P67: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
Adapt
Plot
nu
S
x cuts: xlog Bitmap size:
y cuts: ylog
"-c="

The 2 columns in color are computed by VizieR, and are not part of the original data.
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)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq n a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
151 6C 024105+621506 4.30e+02 8.6e+01 252.00 8893 0 0.03 2.48 041.2604 +62.4625 151 7C 024100.69+621527.00 4.84e+02 9.7e+01 70.20 8893 0 0.03 2.48 041.2404 +62.4683 232 MY 024058.3+622818.8 2.80e+02 6.7e+01 150.00 8893 0 0.02 2.51 041.2304 +62.4719 325 WN B0241.0+6215 3.69e+02 7.4e+01 12.00 8893 0 0.03 2.48 041.2400 +62.4683 365 TXS 0241+622 4.54e+02 9.1e+01 6.00 8893 0 0.03 2.48 041.2414 +62.4683 408 DRAOP 12P67 3.36e+02 6.7e+01 210.00 8893 0 0.03 2.48 041.2496 +62.4686 1400 NVSS J024457+622806 3.64e+02 7.3e+01 45.00 8893 0 0.03 2.48 041.2405 +62.4686 4850 87GB 024100.7+621529 4.05e+02 8.1e+01 138.00 8893 0 0.03 2.48 041.2404 +62.4689 4850 BWE 0241+6215 3.93e+02 7.9e+01 138.00 8893 0 0.02 2.51 041.2388 +62.4697 4850 GB6 B0241+6215 3.76e+02 7.5e+01 108.00 8893 0 0.01 2.55 041.2421 +62.4683 4885 RGB 0244+624 3.76e+02 7.5e+01 4.02 8893 0 0.03 2.48 041.2430 +62.4683 5000 RGB6 J0245.0+6228 4.10e+02 8.2e+01 144.00 8893 0 0.02 2.51 041.2404 +62.4686 10700 RGB2 J0245.0+6228 4.53e+02 9.1e+01 72.00 8893 0 0.03 2.48 041.2404 +62.4686

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)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
74 VLSS J0244.9+6228 7.60e+02 1.5e+02 79.98 -8893 041.2333 +62.4719 151 6C 024105+621506 4.30e+02 8.6e+01 252.00 8893 041.2604 +62.4625 151 7C 024100.69+621527.00 4.84e+02 9.7e+01 70.20 8893 041.2404 +62.4683 232 MY 024058.3+622818.8 2.80e+02 6.7e+01 150.00 8893 041.2304 +62.4719 325 WN B0241.0+6215 3.69e+02 7.4e+01 12.00 8893 041.2400 +62.4683 365 TXS 0241+622 4.54e+02 9.1e+01 6.00 8893 041.2414 +62.4683 408 DRAOP 12P67 3.36e+02 6.7e+01 210.00 8893 041.2496 +62.4686 1400 NVSS J024457+622806 3.64e+02 7.3e+01 45.00 8893 041.2405 +62.4686 1420 CGPSEb 134 9.28e+02 1.9e+02 0.00 -8893 041.1250 +62.2333 2700 F3R 3992 2.10e+02 4.2e+01 150.00 -8893 041.2371 +62.4572 2700 RGB11 J0245.0+6228 2.71e+02 5.4e+01 258.00 -8893 041.2404 +62.4686 4850 87GB 024100.7+621529 4.05e+02 8.1e+01 138.00 8893 041.2404 +62.4689 4850 BWE 0241+6215 3.93e+02 7.9e+01 138.00 8893 041.2388 +62.4697 4885 RGB 0244+624 3.76e+02 7.5e+01 4.02 8893 041.2430 +62.4683 5000 RGB6 J0245.0+6228 4.10e+02 8.2e+01 144.00 8893 041.2404 +62.4686 10700 RGB2 J0245.0+6228 4.53e+02 9.1e+01 72.00 8893 041.2404 +62.4686

Note: For the spectrum finding algorithm, the errors have been increased by 50%