Complement to VIII/85A

Source 6C_070449+815658: 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 J0715.0+8151 5.52e+03 1.1e+03 79.98 103536 0 -0.79 5.23 108.7588 +81.8631 151 6C 070448+815656 3.22e+03 6.4e+02 252.00 103536 0 -0.79 5.23 108.7108 +81.8653 151 6C 070449+815658 3.25e+03 6.5e+02 252.00 103536 0 -0.79 5.23 108.7125 +81.8658 151 7C 070457.50+815649.00 3.33e+03 6.7e+02 70.20 103536 0 -0.79 5.23 108.7471 +81.8633 232 MY 070446.4+815156.5 2.29e+03 4.6e+02 150.00 103536 0 -0.79 5.23 108.7013 +81.8657 325 WN B0704.8+8156 1.70e+03 3.4e+02 12.00 103536 0 -0.79 5.23 108.7103 +81.8650 1400 NVSS J071452+815153 5.51e+02 1.1e+02 45.00 103536 0 -0.79 5.23 108.7167 +81.8649 1400 WB 0704+8156 4.49e+02 9.0e+01 120.00 103536 0 -0.89 5.46 108.5458 +81.8586
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
No object found

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