Complement to VIII/85A

Source 7C_142756.89+402420.00: 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 J1429.9+4011 1.22e+03 2.4e+02 79.98 59883 7 -0.76 4.53 217.4817 +40.1850 151 6C 142757+402432 9.30e+02 1.9e+02 252.00 59883 7 -0.75 4.56 217.4879 +40.1872 151 7C 142756.89+402420.00 7.52e+02 1.5e+02 70.20 59883 7 -0.76 4.53 217.4845 +40.1839 325 WN B1427.9+4024 4.81e+02 9.6e+01 12.00 59883 7 -0.76 4.53 217.4852 +40.1859 365 TXS 1427+404 3.63e+02 7.3e+01 6.00 59883 7 -0.76 4.53 217.4824 +40.1827 408 B3 1427+404 4.10e+02 8.2e+01 84.00 59883 7 -0.76 4.53 217.4892 +40.1847 1400 NVSS J142956+401106 1.62e+02 3.2e+01 45.00 59883 7 -0.76 4.53 217.4845 +40.1853 1400 WB 1427+4024 1.68e+02 3.4e+01 120.00 59883 7 -0.76 4.53 217.4767 +40.1806 4730 B3a 1427+404 5.50e+01 1.1e+01 168.00 59883 7 -0.75 4.56 217.4890 +40.1850 4850 87GB 142754.8+402407 8.75e+01 1.8e+01 138.00 59883 7 -0.81 4.71 217.4762 +40.1803 4850 BWE 1427+4024 6.60e+01 1.3e+01 138.00 59883 7 -0.81 4.71 217.4767 +40.1806 4850 GB6 B1427+4024 5.40e+01 1.1e+01 108.00 59883 7 -0.81 4.71 217.4837 +40.1869 10600 B3VLA 920 2.89e+01 5.8e+00 69.00 59883 7 -0.76 4.53 217.4866 +40.1881

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 J1429.9+4011 1.22e+03 2.4e+02 79.98 59883 217.4817 +40.1850 151 6C 142757+402432 9.30e+02 1.9e+02 252.00 59883 217.4879 +40.1872 151 7C 142756.89+402420.00 7.52e+02 1.5e+02 70.20 59883 217.4845 +40.1839 232 MY 142803.3+401215.5 3.90e+02 1.1e+02 150.00 -59883 217.5112 +40.2043 325 WN B1427.9+4024 4.81e+02 9.6e+01 12.00 59883 217.4852 +40.1859 365 TXS 1427+404 3.63e+02 7.3e+01 6.00 59883 217.4824 +40.1827 408 B3 1427+404 4.10e+02 8.2e+01 84.00 59883 217.4892 +40.1847 1400 FIRST J142952.7+401026 2.20e+00 4.0e-01 5.00 -59883 217.4698 +40.1741 1400 FIRST J142955.5+401126 4.80e+00 9.0e-01 5.00 -59883 217.4816 +40.1907 1400 FIRST J142956.0+401058 9.77e+01 2.0e+01 5.00 -59883 217.4834 +40.1830 1400 FIRST J142957.7+401137 2.42e+01 4.8e+00 5.00 -59883 217.4904 +40.1936 4730 B3a 1427+404 5.50e+01 1.1e+01 168.00 59883 217.4890 +40.1850 4850 87GB 142754.8+402407 8.75e+01 1.8e+01 138.00 59883 217.4762 +40.1803 4850 GB6 B1427+4024 5.40e+01 1.1e+01 108.00 59883 217.4837 +40.1869 10600 B3VLA 920 2.89e+01 5.8e+00 69.00 59883 217.4866 +40.1881

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