Complement to VIII/85A

Source VLA-NEP_J1758.2+6534: 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
74 VLSS J1758.3+6535 1.98e+03 4.3e+02 79.98 75314 1 -0.70 4.62 269.5925 +65.5897 151 6C 175812+653520 1.26e+03 2.5e+02 252.00 75314 1 -0.77 4.73 269.5792 +65.5867 151 7C 175817.30+653543.00 1.13e+03 2.3e+02 70.20 75314 1 -0.77 4.73 269.5992 +65.5933 325 WN B1758.2+6535 7.39e+02 1.5e+02 12.00 75314 1 -0.70 4.62 269.5888 +65.5898 325 WN B1758.2+6535B 5.38e+02 1.1e+02 12.00 75314 1 -0.79 4.77 269.6014 +65.5936 365 TXS 1758+655 6.54e+02 1.3e+02 6.00 75314 1 -0.70 4.62 269.5985 +65.5944 1400 NVSS J175824+653537 1.77e+02 3.5e+01 45.00 75314 1 -0.70 4.62 269.6018 +65.5936 1490 VLA-NEP J1758.2+6534 2.47e+02 4.9e+01 19.98 75314 1 -0.79 4.77 269.5508 +65.5782 1490 VLA-NEP J1758.4+6535 2.26e+02 4.5e+01 19.98 75314 1 -0.79 4.77 269.6028 +65.5936 4850 87GB 175813.6+653520 7.10e+01 1.4e+01 138.00 75314 1 -0.70 4.62 269.5842 +65.5869 4850 GB6 B1758+6535 8.10e+01 1.6e+01 108.00 75314 1 -0.70 4.62 269.5858 +65.5894

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
38 8C 175813+653546 3.30e+03 6.6e+02 270.00 -75314 269.5833 +65.5942 74 VLSS J1758.3+6535 1.98e+03 4.3e+02 79.98 75314 269.5925 +65.5897 151 6C 175812+653520 1.26e+03 2.5e+02 252.00 75314 269.5792 +65.5867 151 7C 175817.30+653543.00 1.13e+03 2.3e+02 70.20 75314 269.5992 +65.5933 232 MY 175815.0+653519.6 6.40e+02 1.3e+02 150.00 -75314 269.5900 +65.5888 325 WN B1758.2+6535 7.39e+02 1.5e+02 12.00 75314 269.5888 +65.5898 325 WN B1758.2+6535A 2.01e+02 4.0e+01 12.00 -75314 269.5519 +65.5788 365 TXS 1758+655 6.54e+02 1.3e+02 6.00 75314 269.5985 +65.5944 1400 NVSS J175812+653443 5.54e+01 1.1e+01 45.00 -75314 269.5521 +65.5788 1400 NVSS J175824+653537 1.77e+02 3.5e+01 45.00 75314 269.6018 +65.5936 1400 WB 1758+6535 2.93e+02 5.9e+01 120.00 -75314 269.5833 +65.5878 1490 VLA-NEP J1758.2+6534 2.47e+02 4.9e+01 19.98 75314 269.5508 +65.5782 1490 VLA-NEP J1758.4+6532 1.00e+00 2.0e-01 19.98 -75314 269.5904 +65.5416 1490 VLA-NEP J1758.4+6535 2.26e+02 4.5e+01 19.98 75314 269.6028 +65.5936 1490 VLA-NEP J1758.5+6536 6.00e-01 2.0e-01 19.98 -75314 269.6293 +65.6127 4850 87GB 175813.6+653520 7.10e+01 1.4e+01 138.00 75314 269.5842 +65.5869 4850 BWE 1758+6535 6.90e+01 1.4e+01 138.00 -75314 269.5833 +65.5878

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