Complement to VIII/85A

Source WB_1445+4615: 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 144512+461508 7.20e+02 1.4e+02 252.00 65200 7 -0.59 4.05 221.7517 +46.0439 151 7C 144515.09+461510.00 6.69e+02 1.3e+02 70.20 65200 7 -0.59 4.05 221.7612 +46.0444 325 WN B1445.2+4615 4.38e+02 8.8e+01 12.00 65200 7 -0.65 4.23 221.7552 +46.0464 408 B3 1445+462 3.30e+02 6.6e+01 84.00 65200 7 -0.68 4.34 221.7571 +46.0472 1400 NVSS J144702+460235 1.25e+02 2.5e+01 45.00 65200 7 -0.60 4.08 221.7621 +46.0432 1400 WB 1445+4615 1.59e+02 3.2e+01 120.00 65200 7 -0.65 4.23 221.7454 +46.0514 4850 BWE 1445+4615 6.40e+01 1.3e+01 138.00 65200 7 -0.65 4.21 221.7454 +46.0514 4850 GB6 B1445+4615 7.50e+01 1.5e+01 108.00 65200 7 -0.65 4.21 221.7529 +46.0481

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 144512+461508 7.20e+02 1.4e+02 252.00 65200 221.7517 +46.0439 232 MY 144513.7+460336.4 3.50e+02 7.0e+01 150.00 -65200 221.7554 +46.0601 325 WN B1445.2+4615 4.38e+02 8.8e+01 12.00 65200 221.7552 +46.0464 408 B3 1445+462 3.30e+02 6.6e+01 84.00 65200 221.7571 +46.0472 1400 FIRST J144649.7+460341 2.30e+00 5.0e-01 5.00 -65200 221.7072 +46.0615 1400 FIRST J144655.6+460309 5.30e+00 1.1e+00 5.00 -65200 221.7318 +46.0527 1400 FIRST J144655.7+460301 7.90e+00 1.6e+00 5.00 -65200 221.7324 +46.0505 1400 FIRST J144656.5+460314 3.64e+01 7.3e+00 5.00 -65200 221.7354 +46.0539 1400 FIRST J144658.5+460354 5.60e+00 1.1e+00 5.00 -65200 221.7441 +46.0652 1400 FIRST J144701.5+460241 5.11e+01 1.0e+01 5.00 -65200 221.7566 +46.0447 1400 FIRST J144703.5+460232 1.77e+01 3.5e+00 5.00 -65200 221.7647 +46.0424 1400 FIRST J144705.3+460221 1.73e+01 3.5e+00 5.00 -65200 221.7724 +46.0394 1400 FIRST J144706.0+460237 1.44e+01 2.9e+00 5.00 -65200 221.7753 +46.0437 1400 FIRST J144711.3+460255 4.10e+00 8.0e-01 5.00 -65200 221.7971 +46.0488 1400 NVSS J144650+460336 3.70e+00 7.0e-01 45.00 -65200 221.7089 +46.0601 1400 NVSS J144656+460311 5.17e+01 1.0e+01 45.00 -65200 221.7342 +46.0532 1400 NVSS J144702+460235 1.25e+02 2.5e+01 45.00 65200 221.7621 +46.0432 1400 WB 1445+4615 1.59e+02 3.2e+01 120.00 65200 221.7454 +46.0514 4850 87GB 144511.2+461537 1.10e+02 2.2e+01 138.00 -65200 221.7454 +46.0519 4850 GB6 B1445+4615 7.50e+01 1.5e+01 108.00 65200 221.7529 +46.0481

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