Complement to VIII/85A

Source FIRST_J170112.3+353353: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
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VIII/85A/spectra
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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
No object foundThe 1 column 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/waste
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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
325 WN B1659.4+3538 6.70e+01 1.3e+01 12.00 -224149 255.3024 +35.5620 1400 FIRST J170111.1+353332 2.50e+00 5.0e-01 5.00 -224149 255.2966 +35.5590 1400 FIRST J170111.2+353338 5.40e+00 1.1e+00 5.00 -224149 255.2970 +35.5608 1400 FIRST J170112.0+353342 3.10e+00 6.0e-01 5.00 -224149 255.3003 +35.5617 1400 FIRST J170112.3+353353 5.40e+01 1.1e+01 5.00 -224149 255.3015 +35.5648 1400 FIRST J170115.4+353303 1.40e+00 3.0e-01 5.00 -224149 255.3143 +35.5509 1400 NVSS J170112+353351 7.07e+01 1.4e+01 45.00 -224149 255.3016 +35.5642 4850 87GB 165923.7+353742 5.87e+01 1.2e+01 138.00 -224149 255.2971 +35.5567 4885 RGB 1701+355 5.00e+01 1.0e+01 4.02 -224149 255.3015 +35.5648 8400 CLASS J170112.3724+353353.432 9.88e+01 2.0e+01 0.33 -224149 255.3015 +35.5648

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