Complement to VIII/85A

Source 6C_171257+501850: 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 J1714.2+5015 9.00e+02 1.8e+02 79.98 78736 0 -1.04 4.98 258.5587 +50.2594 151 6C 171257+501850 4.50e+02 9.0e+01 252.00 78736 0 -0.97 4.77 258.5512 +50.2581 151 6C 171301+501842 5.80e+02 1.2e+02 252.00 78736 0 -0.97 4.77 258.5704 +50.2558 151 7C 171259.70+501853.00 5.23e+02 1.0e+02 70.20 78736 0 -1.04 4.98 258.5608 +50.2589 325 WN B1712.9+5018 2.62e+02 5.2e+01 12.00 78736 0 -0.98 4.78 258.5612 +50.2589 1400 FIRST J171414.7+501530 5.21e+01 1.0e+01 5.00 78736 0 -0.97 4.77 258.5615 +50.2585 1400 NVSS J171414+501530 5.12e+01 1.0e+01 45.00 78736 0 -0.98 4.78 258.5617 +50.2586 1412 WSTB 53W002 5.01e+01 1.0e+01 23.10 78736 0 -0.98 4.78 258.5610 +50.2584
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%