Complement to VIII/85A

Source 87GB_100727.5+414718: 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 100726+414712 8.37e+03 1.7e+03 252.00 41189 0 -0.70 5.42 152.6146 +41.5403 151 7C 100725.89+414711.00 8.71e+03 1.7e+03 70.20 41189 0 -0.70 5.42 152.6137 +41.5400 325 WN B1007.4+4147 4.82e+03 9.6e+02 12.00 41189 0 -0.69 5.40 152.6143 +41.5398 365 TXS 1007+417 4.28e+03 8.6e+02 6.00 41189 0 -0.70 5.42 152.6140 +41.5399 4850 87GB 100727.5+414718 8.82e+02 1.8e+02 138.00 41189 0 -0.69 5.38 152.6204 +41.5419 4850 GB6 B1007+4147 8.54e+02 1.7e+02 108.00 41189 0 -0.70 5.42 152.6183 +41.5417 4885 RGB 1010+415A 8.54e+02 1.7e+02 4.02 41189 0 -0.71 5.46 152.6143 +41.5386 4885 RGB 1010+415B 8.54e+02 1.7e+02 4.02 41189 0 -0.69 5.38 152.6148 +41.5442

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 J1010.4+4132 1.21e+04 2.4e+03 79.98 -41189 152.6146 +41.5417 151 7C 100725.89+414711.00 8.71e+03 1.7e+03 70.20 41189 152.6137 +41.5400 178 4C +41.21 6.30e+03 1.9e+03 690.00 -41189 152.6133 +41.6017 232 MY 100726.3+413217.2 5.66e+03 1.1e+03 150.00 -41189 152.6154 +41.5381 325 WN B1007.4+4147 4.82e+03 9.6e+02 12.00 41189 152.6143 +41.5398 365 TXS 1007+417 4.28e+03 8.6e+02 6.00 41189 152.6140 +41.5399 408 B3 1007+417 4.10e+03 8.2e+02 84.00 -41189 152.6142 +41.5406 1400 FIRST J101027.3+413219 1.18e+03 2.4e+02 5.00 -41189 152.6138 +41.5387 1400 FIRST J101027.5+413238 3.40e+02 6.8e+01 5.00 -41189 152.6147 +41.5441 1400 FIRST J101027.7+413250 9.29e+01 1.9e+01 5.00 -41189 152.6156 +41.5473 1400 NVSS J101027+413236 4.98e+02 1.0e+02 45.00 -41189 152.6151 +41.5435 1400 WB 1007+4147 1.70e+03 3.4e+02 120.00 -41189 152.6213 +41.5419 4730 B3a 1007+417 6.60e+02 1.3e+02 168.00 -41189 152.6143 +41.5406 4850 GB6 B1007+4147 8.54e+02 1.7e+02 108.00 41189 152.6183 +41.5417 4885 RGB 1010+415A 8.54e+02 1.7e+02 4.02 41189 152.6143 +41.5386 4885 RGB 1010+415B 8.54e+02 1.7e+02 4.02 41189 152.6148 +41.5442 5000 RGB6 J1010.5+4132 6.89e+02 1.4e+02 144.00 -41189 152.6213 +41.5417 8400 CLASS J101027.2471+413219.278 1.79e+02 3.6e+01 0.33 -41189 152.6135 +41.5387 8400 CLASS J101027.4326+413218.757 8.13e+01 1.6e+01 0.33 -41189 152.6143 +41.5385 8400 CLASS J101027.5253+413238.957 1.88e+02 3.8e+01 0.33 -41189 152.6147 +41.5442 10600 B3VLA 551 3.35e+02 6.7e+01 69.00 -41189 152.6146 +41.5414

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