Complement to VIII/85A

Source NVSS_J105158+341320: 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 J1051.9+3413 7.63e+03 1.5e+03 79.98 42543 6 -0.85 5.56 162.9938 +34.2225 151 6C 104910+342915 5.15e+03 1.0e+03 252.00 42543 6 -0.80 5.37 162.9921 +34.2219 151 7C 104911.19+342918.00 5.05e+03 1.0e+03 70.20 42543 6 -0.87 5.59 162.9938 +34.2225 232 MY 104910.5+341333.1 3.94e+03 7.9e+02 150.00 42543 6 -0.88 5.62 162.9913 +34.2259 325 WN B1049.1+3429 2.92e+03 5.8e+02 12.00 42543 6 -0.88 5.62 162.9942 +34.2224 325 WN B1049.1+3429A 2.91e+03 5.8e+02 12.00 42543 6 -0.88 5.62 162.9941 +34.2225 365 TXS 1049+344 2.67e+03 5.3e+02 6.00 42543 6 -0.88 5.62 162.9935 +34.2224 408 B2.3 1049+34 2.26e+03 4.5e+02 0.00 42543 6 -0.80 5.37 162.9942 +34.2283 1400 NVSS J105158+341320 7.79e+02 1.6e+02 45.00 42543 6 -0.85 5.56 162.9939 +34.2224 1400 WB 1049+3429 7.32e+02 1.5e+02 120.00 42543 6 -0.91 5.73 162.9863 +34.2258 4850 87GB 104909.2+342929 2.40e+02 4.8e+01 138.00 42543 6 -0.88 5.62 162.9858 +34.2258 4850 BWE 1049+3429 2.36e+02 4.7e+01 138.00 42543 6 -0.88 5.62 162.9863 +34.2258 4850 GB6 B1049+3429 2.15e+02 4.3e+01 108.00 42543 6 -0.85 5.56 162.9888 +34.2256 4850 MITG J105157+3413 2.27e+02 4.5e+01 258.00 42543 6 -0.88 5.62 162.9908 +34.2242

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 J1051.9+3413 7.63e+03 1.5e+03 79.98 42543 162.9938 +34.2225 151 6C 104910+342915 5.15e+03 1.0e+03 252.00 42543 162.9921 +34.2219 178 4C +34.33 3.70e+03 1.1e+03 690.00 -42543 162.9942 +34.2017 232 MY 104910.5+341333.1 3.94e+03 7.9e+02 150.00 42543 162.9913 +34.2259 325 WN B1049.1+3429A 2.91e+03 5.8e+02 12.00 42543 162.9941 +34.2225 325 WN B1049.1+3429B 9.00e+00 3.6e+00 12.00 -42543 163.0340 +34.2169 408 B2.3 1049+34 2.26e+03 4.5e+02 0.00 42543 162.9942 +34.2283 1400 FIRST J105154.3+341325 1.60e+00 3.0e-01 5.00 -42543 162.9764 +34.2239 1400 FIRST J105156.1+341302 2.02e+02 4.0e+01 5.00 -42543 162.9838 +34.2174 1400 FIRST J105156.9+341309 6.68e+01 1.3e+01 5.00 -42543 162.9871 +34.2193 1400 FIRST J105159.5+341327 4.44e+02 8.9e+01 5.00 -42543 162.9981 +34.2244 1400 FIRST J105210.1+341305 1.80e+00 4.0e-01 5.00 -42543 163.0425 +34.2182 4850 87GB 104909.2+342929 2.40e+02 4.8e+01 138.00 42543 162.9858 +34.2258

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