Complement to VIII/85A

Source B3VLA_677: 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
232 MY 113655.7+380343.9 8.30e+02 1.7e+02 150.00 49134 0 -0.54 4.23 174.8933 +38.0622 325 WN B1136.9+3820 1.01e+03 2.0e+02 12.00 49134 0 -0.67 4.68 174.8918 +38.0617 365 TXS 1136+383 1.06e+03 2.1e+02 6.00 49134 0 -0.70 4.82 174.8917 +38.0617 408 B2.3 1136+38 8.17e+02 1.6e+02 0.00 49134 0 -0.66 4.66 174.8954 +38.0550 408 B3 1136+383 8.40e+02 1.7e+02 84.00 49134 0 -0.66 4.66 174.8908 +38.0603 1400 FIRST J113934.0+380342 4.56e+02 9.1e+01 5.00 49134 0 -0.70 4.82 174.8917 +38.0617 1400 NVSS J113934+380342 4.60e+02 9.2e+01 45.00 49134 0 -0.67 4.68 174.8917 +38.0617 1400 WB 1136+3820 4.39e+02 8.8e+01 120.00 49134 0 -0.65 4.64 174.8933 +38.0656 4730 B3a 1136+383 1.77e+02 3.5e+01 168.00 49134 0 -0.67 4.68 174.8908 +38.0604 4850 87GB 113655.7+382033 1.95e+02 3.9e+01 138.00 49134 0 -0.66 4.66 174.8933 +38.0656 4850 BWE 1136+3820 1.92e+02 3.8e+01 138.00 49134 0 -0.66 4.66 174.8933 +38.0656 4850 GB6 B1136+3820 1.81e+02 3.6e+01 108.00 49134 0 -0.67 4.68 174.8929 +38.0631 4850 MITG J113935+3803 1.67e+02 3.3e+01 258.00 49134 0 -0.66 4.66 174.8983 +38.0622 4860 [FPD2001b]a 142 1.78e+02 3.6e+01 0.40 49134 0 -0.70 4.82 174.8916 +38.0616 8460 [FPD2001b]b 142 1.17e+02 2.3e+01 0.20 49134 0 -0.65 4.64 174.8916 +38.0616 10600 B3VLA 677 8.40e+01 1.7e+01 69.00 49134 0 -0.66 4.66 174.8913 +38.0614

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
151 6C 113656+382006 8.30e+02 1.7e+02 252.00 -49134 174.8983 +38.0578 151 7C 113655.10+382018.00 6.09e+02 1.2e+02 70.20 -49134 174.8908 +38.0611 232 MY 113655.7+380343.9 8.30e+02 1.7e+02 150.00 49134 174.8933 +38.0622 325 WN B1136.9+3820 1.01e+03 2.0e+02 12.00 49134 174.8918 +38.0617 408 B2.3 1136+38 8.17e+02 1.6e+02 0.00 49134 174.8954 +38.0550 408 B3 1136+383 8.40e+02 1.7e+02 84.00 49134 174.8908 +38.0603 1400 NVSS J113934+380342 4.60e+02 9.2e+01 45.00 49134 174.8917 +38.0617 1400 WB 1136+3820 4.39e+02 8.8e+01 120.00 49134 174.8933 +38.0656 4730 B3a 1136+383 1.77e+02 3.5e+01 168.00 49134 174.8908 +38.0604 4850 GB6 B1136+3820 1.81e+02 3.6e+01 108.00 49134 174.8929 +38.0631 8460 [FPD2001b]b 142 1.17e+02 2.3e+01 0.20 49134 174.8916 +38.0616 10600 B3VLA 677 8.40e+01 1.7e+01 69.00 49134 174.8913 +38.0614

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