Complement to VIII/104

Source BWE_0620+4556: 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 1 column 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/104/spectra
Post annotation
SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
The parameters of the radio spectra[image] (1658207 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
325 WN B0620.2+4556 1.06e+02 2.1e+01 12.0000 95803 0.12 1.72 095.9860 +45.9121 408 B3 0620+459 1.10e+02 2.2e+01 84.0000 95803 0.12 1.72 095.9817 +45.9119 1400 NVSS J062356+455439 1.28e+02 2.6e+01 45.0000 95803 0.12 1.72 095.9858 +45.9110 4850 87GB 062014.1+455616 2.01e+02 4.0e+01 138.0000 95803 0.12 1.72 095.9854 +45.9111 4850 BWE 0620+4556 1.96e+02 3.9e+01 138.0000 95803 0.12 1.72 095.9858 +45.9108 4850 GB6 B0620+4556 1.94e+02 3.9e+01 108.0000 95803 0.12 1.72 095.9867 +45.9089 8400 CLASS J062356.5105+455439.515 1.57e+02 3.1e+01 0.3300 95803 0.12 1.72 095.9855 +45.9110 8400 CRATES J062356+455432 1.57e+02 3.1e+01 6.0000 95803 0.12 1.72 095.9855 +45.9110 8400 JVAS J0623+459 1.61e+02 3.2e+01 0.3300 95803 0.13 1.70 095.9855 +45.9110
VIII/104/waste
Post annotation
SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
Source parameters based on positional cross-id[spectrum] (3570814 rows)
img(gal)
start AladinLite
No object found

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