Complement to VIII/85A

Source GB6_B2356+4347: 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
178 3CR 470 9.00e+03 1.8e+03 360.00 95491 4 -0.93 6.15 359.6546 +44.1050 178 4C +43.59 9.00e+03 2.7e+03 690.00 95491 4 -0.93 6.15 359.6454 +44.0617 232 MY 235604.1+440423.0 1.25e+04 2.5e+03 150.00 95491 4 -0.94 6.19 359.6546 +44.0731 325 WN B2356.0+4347 6.90e+03 1.4e+03 12.00 95491 4 -0.94 6.19 359.6475 +44.0774 365 TXS 2356+437 5.98e+03 1.2e+03 6.00 95491 4 -0.94 6.19 359.6473 +44.0775 408 B3 2356+437 5.36e+03 1.1e+03 84.00 95491 4 -0.94 6.19 359.6471 +44.0767 1400 NVSS J235835+440440 1.94e+03 3.9e+02 45.00 95491 4 -0.94 6.18 359.6478 +44.0779 1400 WB 2356+4347 1.72e+03 3.4e+02 120.00 95491 4 -0.93 6.15 359.6479 +44.0769 4730 B3a 2356+437 5.38e+02 1.1e+02 168.00 95491 4 -0.94 6.19 359.6472 +44.0768 4850 87GB 235602.2+434755 5.47e+02 1.1e+02 138.00 95491 4 -0.93 6.15 359.6467 +44.0769 4850 BWE 2356+4347 5.45e+02 1.1e+02 138.00 95491 4 -0.93 6.15 359.6479 +44.0769 4850 GB6 B2356+4347 5.42e+02 1.1e+02 108.00 95491 4 -0.93 6.15 359.6479 +44.0753 4850 MITG J235841+4403 4.68e+02 9.4e+01 258.00 95491 4 -0.98 6.30 359.6721 +44.0656 10600 B3VLA 1045 1.86e+02 3.7e+01 69.00 95491 4 -0.93 6.15 359.6500 +44.0800

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 J2358.5+4404 1.86e+04 3.7e+03 79.98 -95491 359.6483 +44.0769 178 4C +43.59 9.00e+03 2.7e+03 690.00 95491 359.6454 +44.0617 232 MY 235604.1+440423.0 1.25e+04 2.5e+03 150.00 95491 359.6546 +44.0731 325 WN B2356.0+4347 6.90e+03 1.4e+03 12.00 95491 359.6475 +44.0774 325 WN B2356.3+4350 3.76e+02 7.5e+01 12.00 -95491 359.7336 +44.1215 325 WN B2356.3+4350B 3.80e+01 7.6e+00 12.00 -95491 359.7448 +44.0992 365 TXS 2356+437 5.98e+03 1.2e+03 6.00 95491 359.6473 +44.0775 408 B3 2356+437 5.36e+03 1.1e+03 84.00 95491 359.6471 +44.0767 408 B3 2356+438 1.90e+02 3.8e+01 84.00 -95491 359.7412 +44.1197 1400 NVSS J235858+440543 4.70e+00 9.0e-01 45.00 -95491 359.7453 +44.0955 1400 WB 2356+4347 1.72e+03 3.4e+02 120.00 95491 359.6479 +44.0769 4730 B3a 2356+437 5.38e+02 1.1e+02 168.00 95491 359.6472 +44.0768 4850 GB6 B2356+4347 5.42e+02 1.1e+02 108.00 95491 359.6479 +44.0753 4850 MITG J235841+4403 4.68e+02 9.4e+01 258.00 95491 359.6721 +44.0656 10600 B3VLA 1045 1.86e+02 3.7e+01 69.00 95491 359.6500 +44.0800

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