Complement to VIII/85A

Source BWE_1714+2308: 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
1400 FIRST J171653.6+230553 3.44e+01 6.9e+00 5.00 73860 0 0.17 1.19 259.2236 +23.0982 1400 NVSS J171653+230553 5.22e+01 1.0e+01 45.00 73860 0 0.17 1.19 259.2240 +23.0982 4850 87GB 171446.6+230837 6.52e+01 1.3e+01 138.00 73860 0 0.17 1.19 259.2183 +23.0903 4850 BWE 1714+2308 4.40e+01 8.8e+00 138.00 73860 0 0.29 0.69 259.2200 +23.0878 4850 GB6 B1714+2309 5.15e+01 1.0e+01 108.00 73860 0 0.40 0.28 259.2217 +23.0972 4850 MITG J171652+2305 6.00e+01 1.2e+01 258.00 73860 0 0.29 0.70 259.2204 +23.0983 4850 MITG J171653+2305 5.80e+01 1.2e+01 258.00 73860 0 0.36 0.45 259.2217 +23.0964 8400 CLASS J171653.6604+230553.299 7.05e+01 1.4e+01 0.33 73860 0 0.29 0.69 259.2236 +23.0981
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%