Complement to VIII/85A

Source WB_0229+3410: 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 J0232.4+3424 2.69e+04 5.4e+03 79.98 8461 5 -0.78 5.90 038.1199 +34.4008 80 Cula 0229+341 2.60e+04 5.2e+03 222.00 8461 5 -0.79 5.90 038.1275 +34.3986 151 7C 022927.30+341049.00 1.45e+04 2.9e+03 70.20 8461 5 -0.78 5.90 038.1204 +34.4006 160 Culb 0229+341 1.81e+04 3.6e+03 111.00 8461 5 -0.79 5.93 038.1275 +34.3986 178 4C +34.08 1.21e+04 3.6e+03 690.00 8461 5 -0.80 5.92 038.1300 +34.4150 232 MY 022926.7+342404.7 1.31e+04 2.6e+03 150.00 8461 5 -0.78 5.90 038.1179 +34.4013 325 WN B0229.4+3410 9.46e+03 1.9e+03 12.00 8461 5 -0.78 5.90 038.1195 +34.4008 365 TXS 0229+341 8.87e+03 1.8e+03 6.00 8461 5 -0.78 5.90 038.1197 +34.4005 408 B2.3 0229+34 6.40e+03 1.3e+03 0.00 8461 5 -0.78 5.90 038.1167 +34.3967 1400 NVSS J023228+342405 2.60e+03 5.2e+02 45.00 8461 5 -0.80 5.92 038.1196 +34.4016 1400 WB 0229+3410 2.68e+03 5.4e+02 120.00 8461 5 -0.82 5.96 038.1158 +34.3989 4850 87GB 022926.1+341043 8.83e+02 1.8e+02 138.00 8461 5 -0.78 5.90 038.1154 +34.3986 4850 BWE 0229+3410 7.53e+02 1.5e+02 138.00 8461 5 -0.78 5.90 038.1158 +34.3989 4850 GB6 B0229+3410 7.95e+02 1.6e+02 108.00 8461 5 -0.79 5.90 038.1183 +34.3997 4850 MITG J023227+3424 8.04e+02 1.6e+02 258.00 8461 5 -0.79 5.93 038.1129 +34.4011

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 J0232.4+3424 2.69e+04 5.4e+03 79.98 8461 038.1199 +34.4008 151 7C 022927.30+341049.00 1.45e+04 2.9e+03 70.20 8461 038.1204 +34.4006 160 Culb 0229+341 1.81e+04 3.6e+03 111.00 8461 038.1275 +34.3986 178 4C +34.08 1.21e+04 3.6e+03 690.00 8461 038.1300 +34.4150 232 MY 022926.7+342404.7 1.31e+04 2.6e+03 150.00 8461 038.1179 +34.4013 325 WN B0229.1+3412A 3.20e+01 6.4e+00 12.00 -8461 038.0495 +34.4237 325 WN B0229.1+3412B 1.60e+01 4.4e+00 12.00 -8461 038.0681 +34.4537 408 B2.3 0229+34 6.40e+03 1.3e+03 0.00 8461 038.1167 +34.3967 1400 NVSS J023212+342533 6.90e+00 1.4e+00 45.00 -8461 038.0527 +34.4259 1400 NVSS J023216+342657 1.20e+01 2.4e+00 45.00 -8461 038.0668 +34.4494 1400 NVSS J023228+342331 2.37e+02 4.7e+01 45.00 -8461 038.1205 +34.3921 1400 NVSS J023229+342307 8.14e+01 1.6e+01 45.00 -8461 038.1217 +34.3855 4850 87GB 022926.1+341043 8.83e+02 1.8e+02 138.00 8461 038.1154 +34.3986

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