Complement to VIII/85A

Source BWE_1630+4424: 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 J1631.5+4418 3.11e+03 6.2e+02 79.98 68621 5 -0.48 4.44 247.8983 +44.3114 151 6C 163003+442500 2.46e+03 4.9e+02 252.00 68621 5 -0.63 4.76 247.9017 +44.3111 151 7C 163001.80+442459.00 2.66e+03 5.3e+02 70.20 68621 5 -0.71 5.03 247.8963 +44.3108 232 MY 163002.0+441836.4 2.18e+03 4.4e+02 150.00 68621 5 -0.71 5.03 247.8971 +44.3101 325 WN B1630.0+4424 1.74e+03 3.5e+02 12.00 68621 5 -0.71 5.02 247.8959 +44.3108 365 TXS 1630+444 1.58e+03 3.2e+02 6.00 68621 5 -0.71 5.03 247.8964 +44.3107 408 B3 1630+444 1.46e+03 2.9e+02 84.00 68621 5 -0.71 5.03 247.8967 +44.3117 1400 NVSS J163135+441839 6.50e+02 1.3e+02 45.00 68621 5 -0.71 5.02 247.8964 +44.3109 1400 WB 1630+4424 6.05e+02 1.2e+02 120.00 68621 5 -0.72 5.04 247.9008 +44.3069 4730 B3a 1630+444 2.51e+02 5.0e+01 168.00 68621 5 -0.63 4.76 247.8965 +44.3118 4850 87GB 163002.7+442445 2.35e+02 4.7e+01 138.00 68621 5 -0.71 5.03 247.9004 +44.3069 4850 BWE 1630+4424 2.04e+02 4.1e+01 138.00 68621 5 -0.72 5.04 247.9008 +44.3069 4850 GB6 B1630+4424 2.10e+02 4.2e+01 108.00 68621 5 -0.71 5.03 247.8983 +44.3089 4850 MITG J163136+4418 2.50e+02 5.0e+01 258.00 68621 5 -0.63 4.76 247.9008 +44.3089

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 J1631.5+4418 3.11e+03 6.2e+02 79.98 68621 247.8983 +44.3114 151 6C 163003+442500 2.46e+03 4.9e+02 252.00 68621 247.9017 +44.3111 151 7C 163001.80+442459.00 2.66e+03 5.3e+02 70.20 68621 247.8963 +44.3108 232 MY 163002.0+441836.4 2.18e+03 4.4e+02 150.00 68621 247.8971 +44.3101 325 WN B1630.0+4424 1.74e+03 3.5e+02 12.00 68621 247.8959 +44.3108 365 TXS 1630+444 1.58e+03 3.2e+02 6.00 68621 247.8964 +44.3107 408 B3 1630+444 1.46e+03 2.9e+02 84.00 68621 247.8967 +44.3117 1400 FIRST J163128.7+441915 8.20e+00 1.6e+00 5.00 -68621 247.8697 +44.3210 1400 FIRST J163134.8+441841 3.14e+02 6.3e+01 5.00 -68621 247.8951 +44.3114 1400 FIRST J163135.3+441837 3.43e+02 6.9e+01 5.00 -68621 247.8973 +44.3104 1400 NVSS J163128+441919 7.20e+00 1.4e+00 45.00 -68621 247.8708 +44.3221 4730 B3a 1630+444 2.51e+02 5.0e+01 168.00 68621 247.8965 +44.3118 4850 GB6 B1630+4424 2.10e+02 4.2e+01 108.00 68621 247.8983 +44.3089 4850 MITG J163136+4418 2.50e+02 5.0e+01 258.00 68621 247.9008 +44.3089

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