Complement to VIII/85A

Source VLSS_J1033.5+5814: 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
38 8C 103021+583016 8.31e+04 1.7e+04 270.00 41930 6 -0.85 6.29 158.3958 +58.2464 74 VLSS J1033.5+5814 4.52e+04 9.0e+03 79.98 41930 6 -0.84 6.25 158.3913 +58.2425 151 6C 103019+583006 2.67e+04 5.3e+03 252.00 41930 6 -0.85 6.29 158.3913 +58.2436 151 7C 103019.60+583004.00 2.67e+04 5.3e+03 70.20 41930 6 -0.84 6.25 158.3917 +58.2431 178 4C +58.21 2.02e+04 6.1e+03 690.00 41930 6 -0.91 6.46 158.3942 +58.2283 232 MY 103019.4+581440.3 1.87e+04 3.7e+03 150.00 41930 6 -0.84 6.25 158.3908 +58.2445 325 WN B1030.3+5829 1.51e+04 3.0e+03 12.00 41930 6 -0.89 6.33 158.3873 +58.2418 325 WN B1030.3+5829B 1.30e+04 2.6e+03 12.00 41930 6 -0.84 6.25 158.3875 +58.2432 365 TXS 1030+585 1.39e+04 2.8e+03 6.00 41930 6 -0.83 6.22 158.3914 +58.2436 1400 NVSS J103333+581437 4.19e+03 8.4e+02 45.00 41930 6 -0.83 6.22 158.3911 +58.2439 1400 WB 1030+5830 4.02e+03 8.0e+02 120.00 41930 6 -0.91 6.40 158.3967 +58.2456 4850 87GB 103020.5+583013 1.27e+03 2.5e+02 138.00 41930 6 -0.84 6.25 158.3954 +58.2456 4850 BWE 1030+5830 1.15e+03 2.3e+02 138.00 41930 6 -0.84 6.25 158.3967 +58.2456 4850 GB6 B1030+5830 1.10e+03 2.2e+02 108.00 41930 6 -0.85 6.29 158.3933 +58.2453

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
38 8C 103021+583016 8.31e+04 1.7e+04 270.00 41930 158.3958 +58.2464 74 VLSS J1033.5+5814 4.52e+04 9.0e+03 79.98 41930 158.3913 +58.2425 151 7C 103019.60+583004.00 2.67e+04 5.3e+03 70.20 41930 158.3917 +58.2431 178 4C +58.21 2.02e+04 6.1e+03 690.00 41930 158.3942 +58.2283 232 MY 103019.4+581440.3 1.87e+04 3.7e+03 150.00 41930 158.3908 +58.2445 325 WN B1030.3+5829 1.51e+04 3.0e+03 12.00 41930 158.3873 +58.2418 325 WN B1030.3+5829A 2.13e+03 4.3e+02 12.00 -41930 158.3855 +58.2327 325 WN B1030.3+5829B 1.30e+04 2.6e+03 12.00 41930 158.3875 +58.2432 1400 FIRST J103333.2+581502 1.47e+03 2.9e+02 5.00 -41930 158.3884 +58.2506 1400 FIRST J103333.5+581453 4.65e+02 9.3e+01 5.00 -41930 158.3898 +58.2483 1400 FIRST J103334.3+581425 6.58e+02 1.3e+02 5.00 -41930 158.3931 +58.2404 1400 FIRST J103334.5+581412 1.25e+03 2.5e+02 5.00 -41930 158.3941 +58.2369 1400 WB 1030+5830 4.02e+03 8.0e+02 120.00 41930 158.3967 +58.2456 4850 GB6 B1030+5830 1.10e+03 2.2e+02 108.00 41930 158.3933 +58.2453

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