Complement to VIII/85A

Source FIRST_J105904.0+160045: 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
365 TXS 1056+162 3.70e+02 7.4e+01 6.00 42812 0 -0.45 3.72 164.7662 +16.0125 1400 FIRST J105904.0+160045 2.09e+02 4.2e+01 5.00 42812 0 -0.48 3.81 164.7669 +16.0127 1400 NVSS J105904+160046 2.02e+02 4.0e+01 45.00 42812 0 -0.48 3.81 164.7670 +16.0128 1400 WB 1056+1617 1.88e+02 3.8e+01 120.00 42812 0 -0.50 3.86 164.7675 +16.0172 4850 87GB 105625.3+161714 9.92e+01 2.0e+01 138.00 42812 0 -0.45 3.72 164.7675 +16.0192 4850 BWE 1056+1617 7.90e+01 1.6e+01 138.00 42812 0 -0.50 3.86 164.7675 +16.0172 4850 GB6 B1056+1617 8.30e+01 1.7e+01 108.00 42812 0 -0.64 4.29 164.7671 +16.0181 4850 MITG J105905+1600 1.06e+02 2.1e+01 258.00 42812 0 -0.45 3.72 164.7713 +16.0014
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%