Complement to VIII/85A

Source FORa_1016+329: 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 J1019.3+3241 3.96e+03 7.9e+02 79.98 41491 4 -0.76 5.18 154.8288 +32.6967 151 6C 101626+325658 2.81e+03 5.6e+02 252.00 41491 4 -0.76 5.18 154.8300 +32.6983 151 7C 101626.80+325653.00 2.96e+03 5.9e+02 70.20 41491 4 -0.72 5.05 154.8296 +32.6969 178 4C +32.35 2.40e+03 7.2e+02 690.00 41491 4 -0.69 4.98 154.8342 +32.6833 232 MY 101626.0+324151.0 2.43e+03 4.9e+02 150.00 41491 4 -0.71 4.99 154.8262 +32.6975 325 WN B1016.4+3256 1.89e+03 3.8e+02 12.00 41491 4 -0.72 5.05 154.8295 +32.6965 365 TXS 1016+329 1.93e+03 3.9e+02 6.00 41491 4 -0.72 5.05 154.8296 +32.6966 408 B2.1 1016+32 1.75e+03 3.5e+02 0.00 41491 4 -0.67 4.91 154.8283 +32.7033 1400 FIRST J101919.4+324142 3.76e+02 7.5e+01 5.00 41491 4 -0.58 4.50 154.8311 +32.6950 1400 NVSS J101919+324148 6.30e+02 1.3e+02 45.00 41491 4 -0.72 5.05 154.8295 +32.6969 1400 WB 1016+3256 6.39e+02 1.3e+02 120.00 41491 4 -0.76 5.18 154.8321 +32.6950 2695 FORa 1016+329 3.49e+02 7.0e+01 286.80 41491 4 -0.72 5.02 154.8275 +32.6956 4750 FORb 1016+329 2.22e+02 4.4e+01 162.60 41491 4 -0.72 5.05 154.8275 +32.6956 4760 [A86] 1016+329 2.15e+02 4.3e+01 168.00 41491 4 -0.75 5.16 154.8275 +32.6956 4850 87GB 101627.2+325646 2.25e+02 4.5e+01 138.00 41491 4 -0.67 4.91 154.8313 +32.6950 4850 BWE 1016+3256 2.23e+02 4.5e+01 138.00 41491 4 -0.72 5.05 154.8321 +32.6950 4850 GB6 B1016+3256 2.11e+02 4.2e+01 108.00 41491 4 -0.67 4.91 154.8308 +32.6931 4850 MITG J101917+3241 2.41e+02 4.8e+01 258.00 41491 4 -0.67 4.91 154.8217 +32.6950

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
151 6C 101626+325658 2.81e+03 5.6e+02 252.00 41491 154.8300 +32.6983 178 4C +32.35 2.40e+03 7.2e+02 690.00 41491 154.8342 +32.6833 325 WN B1016.1+3253 1.90e+01 3.8e+00 12.00 -41491 154.7574 +32.6485 408 B2.1 1016+32 1.75e+03 3.5e+02 0.00 41491 154.8283 +32.7033 1400 FIRST J101914.4+324330 9.00e-01 2.0e-01 5.00 -41491 154.8101 +32.7251 1400 FIRST J101923.7+324411 7.00e-01 1.0e-01 5.00 -41491 154.8491 +32.7365 1400 FIRST J101927.0+324154 2.20e+00 4.0e-01 5.00 -41491 154.8628 +32.6985 1400 NVSS J101901+323905 9.10e+00 1.8e+00 45.00 -41491 154.7579 +32.6516 4850 MITG J101917+3241 2.41e+02 4.8e+01 258.00 41491 154.8217 +32.6950

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