Complement to VIII/85A

Source CLASS_J174232.0073+594506.729: 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
325 WN B1741.8+5946 1.01e+02 2.0e+01 12.00 74735 0 0.03 1.92 265.6305 +59.7524 1400 FIRST J174231.9+594506 1.25e+02 2.5e+01 5.00 74735 0 -0.05 2.13 265.6332 +59.7518 1400 NVSS J174231+594507 1.06e+02 2.1e+01 45.00 74735 0 -0.05 2.13 265.6332 +59.7520 4850 87GB 174152.6+594621 9.00e+01 1.8e+01 138.00 74735 0 0.03 1.92 265.6342 +59.7508 4850 BWE 1741+5946 8.70e+01 1.7e+01 138.00 74735 0 0.03 1.92 265.6346 +59.7503 4850 GB6 B1741+5946 8.80e+01 1.8e+01 108.00 74735 0 0.03 1.92 265.6300 +59.7536 4885 RGB 1742+597 8.80e+01 1.8e+01 4.02 74735 0 0.03 1.92 265.6333 +59.7519 8400 CLASS J174232.0073+594506.729 1.16e+02 2.3e+01 0.33 74735 0 0.03 1.92 265.6333 +59.7519
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%