Complement to VIII/85A

Source BWE_2156+5408: 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
38 8C 215634+540857 1.59e+04 3.2e+03 270.00 89021 5 -1.16 5.95 329.5833 +54.3886 178 4C +54.45 2.20e+03 6.6e+02 690.00 89021 5 -0.97 5.49 329.5842 +54.3583 325 WN B2156.5+5407 1.10e+03 2.2e+02 12.00 89021 5 -0.98 5.51 329.5755 +54.3684 365 TXS 2156+541 7.72e+02 1.5e+02 6.00 89021 5 -1.16 5.95 329.5790 +54.3709 1400 NVSS J215818+542217 2.66e+02 5.3e+01 45.00 89021 5 -0.98 5.51 329.5766 +54.3714 1400 WB 2156+5408 2.49e+02 5.0e+01 120.00 89021 5 -0.98 5.51 329.5783 +54.3775 1410 RRF 942 2.04e+02 4.1e+01 564.00 89021 5 -0.97 5.49 329.5542 +54.3686 4850 87GB 215632.1+540820 8.50e+01 1.7e+01 138.00 89021 5 -0.97 5.49 329.5775 +54.3783 4850 BWE 2156+5408 8.30e+01 1.7e+01 138.00 89021 5 -0.97 5.49 329.5783 +54.3775 4850 GB6 B2156+5408 8.20e+01 1.6e+01 108.00 89021 5 -0.97 5.49 329.5775 +54.3781

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 215634+540857 1.59e+04 3.2e+03 270.00 89021 329.5833 +54.3886 74 VLSS J2158.2+5421 4.87e+03 9.7e+02 79.98 -89021 329.5700 +54.3667 178 4C +54.45 2.20e+03 6.6e+02 690.00 89021 329.5842 +54.3583 232 MY 215633.9+542155.2 8.50e+02 2.4e+02 150.00 -89021 329.5850 +54.3653 232 MY 215636.1+542204.3 1.59e+03 3.2e+02 150.00 -89021 329.5942 +54.3679 325 WN B2156.5+5407 1.10e+03 2.2e+02 12.00 89021 329.5755 +54.3684 365 TXS 2156+541 7.72e+02 1.5e+02 6.00 89021 329.5790 +54.3709 1400 GPSR 099.391-0.391 9.60e+01 1.9e+01 5.00 -89021 329.5780 +54.3694 1400 GPSR 099.394-0.386 1.11e+02 2.2e+01 5.00 -89021 329.5762 +54.3749 1400 NVSS J215816+542121 1.13e+01 2.3e+00 45.00 -89021 329.5670 +54.3560 1400 WB 2156+5408 2.49e+02 5.0e+01 120.00 89021 329.5783 +54.3775 1400 [WBH2005] G99.389-0.393 1.09e+01 2.2e+00 6.00 -89021 329.5776 +54.3665 1400 [WBH2005] G99.391-0.391 7.55e+01 1.5e+01 6.00 -89021 329.5783 +54.3695 1400 [WBH2005] G99.394-0.385 7.46e+01 1.5e+01 6.00 -89021 329.5759 +54.3753 1400 [WBH2005] G99.394-0.388 9.00e+00 1.8e+00 6.00 -89021 329.5789 +54.3734 1410 RRF 942 2.04e+02 4.1e+01 564.00 89021 329.5542 +54.3686 2700 F3R 3140 1.50e+02 3.0e+01 150.00 -89021 329.5883 +54.3775 4850 BWE 2156+5408 8.30e+01 1.7e+01 138.00 89021 329.5783 +54.3775 4850 GB6 B2156+5408 8.20e+01 1.6e+01 108.00 89021 329.5775 +54.3781

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