Complement to VIII/85A

Source 6C_110550+391507: 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 J1108.5+3858 7.90e+03 1.6e+03 79.98 48141 5 -0.83 5.53 167.1500 +38.9831 151 6C 110550+391507 5.18e+03 1.0e+03 252.00 48141 5 -0.81 5.41 167.1513 +38.9808 151 7C 110550.29+391508.00 5.08e+03 1.0e+03 70.20 48141 5 -0.83 5.53 167.1517 +38.9811 178 4C +39.34 3.70e+03 1.1e+03 690.00 48141 5 -0.81 5.41 167.1513 +39.0017 232 MY 110549.9+385846.3 2.52e+03 5.0e+02 150.00 48141 5 -0.81 5.41 167.1504 +38.9795 325 WN B1105.8+3915 2.90e+03 5.8e+02 12.00 48141 5 -0.81 5.41 167.1520 +38.9820 365 TXS 1105+392 3.49e+03 7.0e+02 6.00 48141 5 -0.83 5.53 167.1502 +38.9803 408 B2.3 1105+39 2.58e+03 5.2e+02 0.00 48141 5 -0.83 5.51 167.1525 +38.9833 408 B3 1105+392 2.31e+03 4.6e+02 84.00 48141 5 -0.81 5.41 167.1525 +38.9839 1400 FIRST J110836.0+385900 6.56e+02 1.3e+02 5.00 48141 5 -0.81 5.41 167.1501 +38.9834 1400 NVSS J110836+385858 8.41e+02 1.7e+02 45.00 48141 5 -0.83 5.53 167.1504 +38.9828 1400 WB 1105+3915 9.30e+02 1.9e+02 120.00 48141 5 -0.85 5.57 167.1612 +38.9878 4850 87GB 110552.7+391533 3.13e+02 6.3e+01 138.00 48141 5 -0.83 5.53 167.1617 +38.9883 4850 BWE 1105+3915 2.63e+02 5.3e+01 138.00 48141 5 -0.83 5.53 167.1612 +38.9878 4850 GB6 B1105+3915 2.69e+02 5.4e+01 108.00 48141 5 -0.81 5.41 167.1538 +38.9844 10600 B3VLA 635 1.28e+02 2.6e+01 69.00 48141 5 -0.83 5.51 167.1579 +38.9775

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 J1108.5+3858 7.90e+03 1.6e+03 79.98 48141 167.1500 +38.9831 151 6C 110550+391507 5.18e+03 1.0e+03 252.00 48141 167.1513 +38.9808 178 4C +39.34 3.70e+03 1.1e+03 690.00 48141 167.1513 +39.0017 232 MY 110549.9+385846.3 2.52e+03 5.0e+02 150.00 48141 167.1504 +38.9795 325 WN B1105.8+3915 2.90e+03 5.8e+02 12.00 48141 167.1520 +38.9820 365 TXS 1105+392 3.49e+03 7.0e+02 6.00 48141 167.1502 +38.9803 408 B2.3 1105+39 2.58e+03 5.2e+02 0.00 48141 167.1525 +38.9833 1400 FIRST J110836.2+385854 1.30e+02 2.6e+01 5.00 -48141 167.1512 +38.9817 1400 FIRST J110839.5+385825 4.70e+01 9.4e+00 5.00 -48141 167.1648 +38.9737 4730 B3a 1105+392 2.95e+02 5.9e+01 168.00 -48141 167.1521 +38.9841 4850 GB6 B1105+3915 2.69e+02 5.4e+01 108.00 48141 167.1538 +38.9844 10600 B3VLA 635 1.28e+02 2.6e+01 69.00 48141 167.1579 +38.9775

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