Complement to VIII/85A

Source GB6_B0944+0957: 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 J0947.0+0943 9.80e+02 2.0e+02 79.98 40397 6 -0.60 4.12 146.7646 +09.7269 1400 NVSS J094702+094336 1.66e+02 3.3e+01 45.00 40397 6 -0.56 4.03 146.7612 +09.7269 1400 WB 0944+0957 1.44e+02 2.9e+01 120.00 40397 6 -0.67 4.24 146.7675 +09.7225 4850 87GB 094424.0+095725 9.39e+01 1.9e+01 138.00 40397 6 -0.60 4.12 146.7675 +09.7250 4850 BWE 0944+0957 6.00e+01 1.2e+01 138.00 40397 6 -0.65 4.21 146.7675 +09.7225 4850 GB6 B0944+0957 7.58e+01 1.5e+01 108.00 40397 6 -0.61 4.14 146.7688 +09.7250 4850 MITG J094703+0943 9.50e+01 1.9e+01 258.00 40397 6 -0.60 4.12 146.7629 +09.7256 4850 PMN J0947+0943 5.50e+01 1.1e+01 168.00 40397 6 -0.65 4.21 146.7658 +09.7300

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 J0947.0+0943 9.80e+02 2.0e+02 79.98 40397 146.7646 +09.7269 611 NAIC 0944+099 3.82e+02 1.3e+02 756.00 -40397 146.7862 +09.7517 1400 FIRST J094641.7+094708 8.00e-01 2.0e-01 5.00 -40397 146.6739 +09.7858 1400 FIRST J094646.7+094606 3.10e+00 6.0e-01 5.00 -40397 146.6947 +09.7684 1400 FIRST J094652.8+094832 1.40e+00 3.0e-01 5.00 -40397 146.7203 +09.8091 1400 FIRST J094702.1+094320 7.67e+01 1.5e+01 5.00 -40397 146.7591 +09.7224 1400 FIRST J094703.2+094401 7.06e+01 1.4e+01 5.00 -40397 146.7635 +09.7339 1400 FIRST J094708.5+094506 5.40e+00 1.1e+00 5.00 -40397 146.7856 +09.7519 1400 FIRST J094709.8+094504 3.00e+00 6.0e-01 5.00 -40397 146.7910 +09.7511 1400 FIRST J094710.8+094503 6.60e+00 1.3e+00 5.00 -40397 146.7951 +09.7508 1400 FIRST J094714.1+094806 8.20e+00 1.6e+00 5.00 -40397 146.8091 +09.8019 1400 FIRST J094715.7+094445 4.90e+00 1.0e+00 5.00 -40397 146.8156 +09.7460 1400 FIRST J094729.1+094836 1.70e+00 3.0e-01 5.00 -40397 146.8716 +09.8103 1400 FIRST J094733.0+094402 9.30e+00 1.9e+00 5.00 -40397 146.8878 +09.7339 1400 NVSS J094702+094336 1.66e+02 3.3e+01 45.00 40397 146.7612 +09.7269 1400 NVSS J094709+094505 2.05e+01 4.1e+00 45.00 -40397 146.7894 +09.7515 1400 NVSS J094729+094829 2.80e+00 6.0e-01 45.00 -40397 146.8717 +09.8082 1400 WB 0944+0957 1.44e+02 2.9e+01 120.00 40397 146.7675 +09.7225 4850 MITG J094703+0943 9.50e+01 1.9e+01 258.00 40397 146.7629 +09.7256 4850 PMN J0947+0943 5.50e+01 1.1e+01 168.00 40397 146.7658 +09.7300

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