Complement to VIII/85A

Source VLSS_J1128.2+2251: 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
74 VLSS J1128.2+2251 8.50e+02 1.7e+02 79.98 48756 0 -0.47 3.80 172.0613 +22.8651 1400 NVSS J112814+225152 1.82e+02 3.6e+01 45.00 48756 0 -0.47 3.80 172.0624 +22.8647 1400 WB 1125+2308 1.91e+02 3.8e+01 120.00 48756 0 -0.47 3.80 172.0629 +22.8725 2700 RGB11 J1128.2+2251 1.41e+02 2.8e+01 258.00 48756 0 -0.49 3.83 172.0629 +22.8722 4850 87GB 112537.2+230853 1.82e+02 3.6e+01 138.00 48756 0 -0.53 3.95 172.0625 +22.8728 4850 BWE 1125+2308 1.42e+02 2.8e+01 138.00 48756 0 -0.47 3.80 172.0629 +22.8725 4850 GB6 B1125+2308 1.46e+02 2.9e+01 108.00 48756 0 -0.47 3.80 172.0633 +22.8672 4850 MITG J112814+2252 1.27e+02 2.5e+01 258.00 48756 0 -0.53 3.95 172.0613 +22.8681 4885 RGB 1128+228 1.46e+02 2.9e+01 4.02 48756 0 -0.47 3.80 172.0615 +22.8636 5000 RGB6 J1128.2+2251 1.19e+02 2.4e+01 144.00 48756 0 -0.49 3.83 172.0629 +22.8722 8400 CLASS J112814.7475+225148.939 7.72e+01 1.5e+01 0.33 48756 0 -0.47 3.80 172.0614 +22.8636 8400 JVAS J1128+2251 7.38e+01 1.5e+01 0.33 48756 0 -0.49 3.83 172.0615 +22.8636 10700 RGB2 J1128.2+2251 7.00e+01 1.4e+01 72.00 48756 0 -0.47 3.80 172.0629 +22.8722

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/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

nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
74 VLSS J1128.2+2251 8.50e+02 1.7e+02 79.98 48756 172.0613 +22.8651 1400 FIRST J112814.0+225132 5.50e+00 1.1e+00 5.00 -48756 172.0584 +22.8591 1400 FIRST J112814.7+225149 1.02e+02 2.0e+01 5.00 -48756 172.0614 +22.8636 1400 FIRST J112815.1+225158 2.03e+01 4.1e+00 5.00 -48756 172.0632 +22.8663 1400 FIRST J112815.6+225210 3.47e+01 6.9e+00 5.00 -48756 172.0651 +22.8695 1400 NVSS J112814+225152 1.82e+02 3.6e+01 45.00 48756 172.0624 +22.8647 1400 WB 1125+2308 1.91e+02 3.8e+01 120.00 48756 172.0629 +22.8725 4850 87GB 112537.2+230853 1.82e+02 3.6e+01 138.00 48756 172.0625 +22.8728 4850 GB6 B1125+2308 1.46e+02 2.9e+01 108.00 48756 172.0633 +22.8672 4850 MITG J112814+2252 1.27e+02 2.5e+01 258.00 48756 172.0613 +22.8681 4885 RGB 1128+228 1.46e+02 2.9e+01 4.02 48756 172.0615 +22.8636 5000 RGB6 J1128.2+2251 1.19e+02 2.4e+01 144.00 48756 172.0629 +22.8722 8400 CLASS J112814.7475+225148.939 7.72e+01 1.5e+01 0.33 48756 172.0614 +22.8636 8400 JVAS J1128+2251 7.38e+01 1.5e+01 0.33 48756 172.0615 +22.8636

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