Complement to VIII/85A

Source 4C_+71.09: 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
151 6C 100725+713931 4.02e+03 8.0e+02 252.00 100243 4 -0.55 4.94 152.8837 +71.4119 151 7C 100726.39+713928.00 4.49e+03 9.0e+02 70.20 100243 4 -0.55 4.94 152.8870 +71.4111 178 4C +71.09 5.00e+03 1.5e+03 690.00 100243 4 -0.62 5.19 152.8762 +71.4350 232 MY 100725.8+712448.2 6.07e+03 1.2e+03 150.00 100243 4 -0.62 5.19 152.8846 +71.4134 325 WN B1007.4+7139 4.31e+03 8.6e+02 12.00 100243 4 -0.62 5.19 152.8877 +71.4113 1400 NVSS J101132+712440 1.96e+03 3.9e+02 45.00 100243 4 -0.60 5.15 152.8861 +71.4113 1400 WB 1007+7139 1.89e+03 3.8e+02 120.00 100243 4 -0.62 5.19 152.8833 +71.4081 2700 RGB11 J1011.5+7124 1.20e+03 2.4e+02 258.00 100243 4 -0.62 5.19 152.8829 +71.4078 4850 87GB 100725.5+713916 8.64e+02 1.7e+02 138.00 100243 4 -0.62 5.19 152.8833 +71.4078 4850 BWE 1007+7139 7.70e+02 1.5e+02 138.00 100243 4 -0.64 5.23 152.8833 +71.4081 4850 GB6 B1007+7139 7.53e+02 1.5e+02 108.00 100243 4 -0.64 5.25 152.8833 +71.4094 4885 RGB 1011+714 7.53e+02 1.5e+02 4.02 100243 4 -0.58 4.84 152.8859 +71.4116 5000 RGB6 J1011.5+7124 7.95e+02 1.6e+02 144.00 100243 4 -0.60 5.15 152.8829 +71.4078 10700 RGB2 J1011.5+7124 2.84e+02 5.7e+01 72.00 100243 4 -0.58 4.84 152.8829 +71.4078

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 J1011.5+7124 1.59e+03 3.2e+02 79.98 -100243 152.8892 +71.4119 151 6C 100725+713931 4.02e+03 8.0e+02 252.00 100243 152.8837 +71.4119 151 7C 100726.39+713928.00 4.49e+03 9.0e+02 70.20 100243 152.8870 +71.4111 178 4C +71.09 5.00e+03 1.5e+03 690.00 100243 152.8762 +71.4350 232 MY 100725.8+712448.2 6.07e+03 1.2e+03 150.00 100243 152.8846 +71.4134 325 WN B1006.4+7141 4.70e+01 9.4e+00 12.00 -100243 152.6343 +71.4420 325 WN B1007.4+7139 4.31e+03 8.6e+02 12.00 100243 152.8877 +71.4113 1400 NVSS J101031+712629 1.44e+01 2.9e+00 45.00 -100243 152.6294 +71.4415 1400 WB 1007+7139 1.89e+03 3.8e+02 120.00 100243 152.8833 +71.4081 4850 87GB 100725.5+713916 8.64e+02 1.7e+02 138.00 100243 152.8833 +71.4078 4885 RGB 1011+714 7.53e+02 1.5e+02 4.02 100243 152.8859 +71.4116 5000 RGB6 J1011.5+7124 7.95e+02 1.6e+02 144.00 100243 152.8829 +71.4078 8400 CLASS J101132.6159+712441.615 3.72e+02 7.4e+01 0.33 -100243 152.8859 +71.4116

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