Complement to VIII/85A

Source PMN_J1508+0415: 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 J150759.7+041512 1.85e+02 3.7e+01 5.00 106710 0 -0.05 2.43 226.9989 +04.2534 1400 NVSS J150759+041512 1.67e+02 3.3e+01 45.00 106710 0 0.01 2.20 226.9988 +04.2536 4850 87GB 150529.4+042615 2.29e+02 4.6e+01 138.00 106710 0 -0.05 2.43 226.9979 +04.2467 4850 BWE 1505+0426 2.23e+02 4.5e+01 138.00 106710 0 -0.05 2.43 227.0000 +04.2467 4850 GB6 B1505+0426 2.40e+02 4.8e+01 108.00 106710 0 -0.05 2.43 226.9992 +04.2550 4850 MITG J150800+0415 1.74e+02 3.5e+01 258.00 106710 0 -0.05 2.43 227.0000 +04.2583 4850 PMN J1508+0415 2.36e+02 4.7e+01 168.00 106710 0 -0.05 2.43 227.0017 +04.2522 8400 JVAS J1507+0415 1.69e+02 3.4e+01 0.33 106710 0 -0.05 2.43 226.9989 +04.2533
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%