Complement to VIII/85A

Source WN_B0210.9+5131: 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
325 WN B0210.9+5131 6.54e+02 1.3e+02 12.00 7799 0 -0.30 3.57 033.5678 +51.7528 325 WN B0210.9+5131B 4.70e+02 9.4e+01 12.00 7799 0 -0.36 3.67 033.5755 +51.7478 365 TXS 0210+515 5.65e+02 1.1e+02 6.00 7799 0 -0.28 3.46 033.5742 +51.7477 1400 WB 0210+5131 4.90e+02 9.8e+01 120.00 7799 0 -0.36 3.67 033.5721 +51.7547 2700 RGB11 J0214.3+5144 3.44e+02 6.9e+01 258.00 7799 0 -0.36 3.67 033.5721 +51.7547 4850 87GB 021057.1+513119 3.10e+02 6.2e+01 138.00 7799 0 -0.36 3.78 033.5708 +51.7550 4850 BWE 0210+5131 2.71e+02 5.4e+01 138.00 7799 0 -0.28 3.48 033.5721 +51.7547 4850 GB6 B0210+5131 2.91e+02 5.8e+01 108.00 7799 0 -0.28 3.46 033.5725 +51.7539 4885 RGB 0214+517 2.91e+02 5.8e+01 4.02 7799 0 -0.28 3.46 033.5748 +51.7478 5000 RGB6 J0214.3+5144 2.73e+02 5.5e+01 144.00 7799 0 -0.36 3.67 033.5721 +51.7547 8400 CLASS J021417.9334+514451.953 1.62e+02 3.2e+01 0.33 7799 0 -0.28 3.46 033.5747 +51.7478 8400 JVAS J0214+517 1.68e+02 3.4e+01 0.33 7799 0 -0.36 3.67 033.5747 +51.7478 10700 RGB2 J0214.3+5144 1.96e+02 3.9e+01 72.00 7799 0 -0.28 3.46 033.5721 +51.7547

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
151 6C 021056+513115 9.70e+02 1.9e+02 252.00 -7799 033.5679 +51.7539 232 MY 021057.5+514522.7 4.60e+02 9.2e+01 150.00 -7799 033.5725 +51.7563 325 WN B0210.9+5131A 1.83e+02 3.7e+01 12.00 -7799 033.5405 +51.7686 325 WN B0210.9+5131B 4.70e+02 9.4e+01 12.00 7799 033.5755 +51.7478 325 WN B0210.9+5131 6.54e+02 1.3e+02 12.00 7799 033.5678 +51.7528 365 TXS 0210+515 5.65e+02 1.1e+02 6.00 7799 033.5742 +51.7477 1400 NVSS J021424+514505 3.49e+01 7.0e+00 45.00 -7799 033.6031 +51.7515 1400 NVSS J021418+514452 2.94e+02 5.9e+01 45.00 -7799 033.5750 +51.7479 1400 NVSS J021409+514610 1.21e+02 2.4e+01 45.00 -7799 033.5392 +51.7696 1400 NVSS J021421+514637 3.20e+00 6.0e-01 45.00 -7799 033.5892 +51.7769 4850 87GB 021057.1+513119 3.10e+02 6.2e+01 138.00 7799 033.5708 +51.7550 4850 GB6 B0210+5131 2.91e+02 5.8e+01 108.00 7799 033.5725 +51.7539 4885 RGB 0214+517 2.91e+02 5.8e+01 4.02 7799 033.5748 +51.7478 5000 RGB6 J0214.3+5144 2.73e+02 5.5e+01 144.00 7799 033.5721 +51.7547 8400 CLASS J021417.9334+514451.953 1.62e+02 3.2e+01 0.33 7799 033.5747 +51.7478

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


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