Complement to VIII/85A

Source 87GB_132042.1+295714: 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 J1323.0+2941 8.37e+03 1.7e+03 79.98 57772 4 -0.67 5.20 200.7608 +29.6917 80 Cula 1320+299 1.20e+04 2.4e+03 222.00 57772 4 -0.74 5.46 200.7675 +29.6922 160 Culb 1320+299 6.80e+03 1.4e+03 111.00 57772 4 -0.75 5.51 200.7675 +29.6922 325 WN B1320.7+2957 4.34e+03 8.7e+02 12.00 57772 4 -0.67 5.20 200.7602 +29.6919 365 TXS 1320+299 3.91e+03 7.8e+02 6.00 57772 4 -0.69 5.32 200.7598 +29.6929 408 B2.1 1320+29 3.22e+03 6.4e+02 0.00 57772 4 -0.69 5.32 200.7583 +29.6917 1400 NVSS J132302+294134 1.37e+03 2.7e+02 45.00 57772 4 -0.69 5.32 200.7597 +29.6928 1400 WB 1320+2957 1.27e+03 2.5e+02 120.00 57772 4 -0.69 5.30 200.7608 +29.6939 4850 87GB 132042.1+295714 6.63e+02 1.3e+02 138.00 57772 4 -0.69 5.32 200.7604 +29.6931 4850 BWE 1320+2957 5.88e+02 1.2e+02 138.00 57772 4 -0.69 5.30 200.7608 +29.6939 4850 GB6 B1320+2957 5.54e+02 1.1e+02 108.00 57772 4 -0.64 5.12 200.7583 +29.6919 4850 MITG J132302+2941 6.02e+02 1.2e+02 258.00 57772 4 -0.69 5.32 200.7608 +29.6914

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 J1323.0+2941 8.37e+03 1.7e+03 79.98 57772 200.7608 +29.6917 160 Culb 1320+299 6.80e+03 1.4e+03 111.00 57772 200.7675 +29.6922 178 4C +29.48 4.00e+03 1.2e+03 690.00 -57772 200.7617 +29.7233 325 WN B1320.7+2957 4.34e+03 8.7e+02 12.00 57772 200.7602 +29.6919 408 B2.1 1320+29 3.22e+03 6.4e+02 0.00 57772 200.7583 +29.6917 1400 FIRST J132256.3+294028 2.60e+00 5.0e-01 5.00 -57772 200.7347 +29.6746 1400 FIRST J132257.4+294125 7.00e-01 2.0e-01 5.00 -57772 200.7393 +29.6904 1400 FIRST J132258.3+294216 1.40e+00 3.0e-01 5.00 -57772 200.7431 +29.7045 1400 FIRST J132258.8+294301 2.60e+00 5.0e-01 5.00 -57772 200.7451 +29.7170 1400 FIRST J132259.5+294303 2.30e+00 5.0e-01 5.00 -57772 200.7482 +29.7176 1400 FIRST J132259.7+294203 3.20e+00 6.0e-01 5.00 -57772 200.7491 +29.7010 1400 FIRST J132300.8+294144 4.40e+02 8.8e+01 5.00 -57772 200.7537 +29.6958 1400 FIRST J132301.5+294243 7.00e-01 2.0e-01 5.00 -57772 200.7566 +29.7120 1400 FIRST J132302.5+294133 7.14e+02 1.4e+02 5.00 -57772 200.7608 +29.6926 1400 FIRST J132304.1+294115 2.58e+02 5.2e+01 5.00 -57772 200.7672 +29.6876 4850 GB6 B1320+2957 5.54e+02 1.1e+02 108.00 57772 200.7583 +29.6919

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