Complement to VIII/85A

Source GB6_B0835+6431: 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 J0840.1+6420 8.40e+02 1.7e+02 79.98 38362 1 -0.78 4.39 130.0421 +64.3428 325 WN B0835.8+6431 4.11e+02 8.2e+01 12.00 38362 1 -0.40 3.61 130.0418 +64.3401 325 WN B0835.8+6431B 2.31e+02 4.6e+01 12.00 38362 1 -0.78 4.39 130.0538 +64.3467 1400 FIRST J084013.1+642052 9.32e+01 1.9e+01 5.00 38362 1 -0.77 4.34 130.0549 +64.3478 1400 NVSS J084013+642051 9.31e+01 1.9e+01 45.00 38362 1 -0.77 4.33 130.0550 +64.3477 1400 WB 0835+6431 2.46e+02 4.9e+01 120.00 38362 1 -0.40 3.61 130.0475 +64.3403 4850 87GB 083549.7+643102 1.55e+02 3.1e+01 138.00 38362 1 -0.18 2.82 130.0462 +64.3403 4850 GB6 B0835+6431 1.41e+02 2.8e+01 108.00 38362 1 -0.40 3.61 130.0442 +64.3408 8400 CLASS J084013.1572+642051.453 2.07e+01 4.1e+00 0.33 38362 1 -0.78 4.39 130.0548 +64.3476

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 J0840.1+6420 8.40e+02 1.7e+02 79.98 38362 130.0421 +64.3428 151 7C 083550.60+643124.00 4.53e+02 9.1e+01 70.20 -38362 130.0504 +64.3461 325 WN B0835.8+6431 4.11e+02 8.2e+01 12.00 38362 130.0418 +64.3401 325 WN B0835.8+6431B 2.31e+02 4.6e+01 12.00 38362 130.0538 +64.3467 365 TXS 0835+645 3.39e+02 6.8e+01 6.00 -38362 130.0234 +64.3321 1400 FIRST J084013.1+642052 9.32e+01 1.9e+01 5.00 38362 130.0549 +64.3478 1400 NVSS J084013+642051 9.31e+01 1.9e+01 45.00 38362 130.0550 +64.3477 1400 WB 0835+6431 2.46e+02 4.9e+01 120.00 38362 130.0475 +64.3403 4850 87GB 083549.7+643102 1.55e+02 3.1e+01 138.00 38362 130.0462 +64.3403 4850 GB6 B0835+6431 1.41e+02 2.8e+01 108.00 38362 130.0442 +64.3408 8400 CLASS J084002.8267+642028.518 9.00e-01 2.0e-01 0.33 -38362 130.0118 +64.3413 8400 CLASS J084008.5327+641926.225 9.00e-01 2.0e-01 0.33 -38362 130.0355 +64.3239 8400 CLASS J084010.1085+641954.460 4.00e-01 1.0e-01 0.33 -38362 130.0421 +64.3318 8400 CLASS J084010.9736+642011.269 1.40e+00 3.0e-01 0.33 -38362 130.0457 +64.3365 8400 CLASS J084011.2861+642010.637 1.40e+00 3.0e-01 0.33 -38362 130.0470 +64.3363 8400 CLASS J084011.7222+642022.832 3.90e+00 8.0e-01 0.33 -38362 130.0488 +64.3397 8400 CLASS J084013.1572+642051.453 2.07e+01 4.1e+00 0.33 38362 130.0548 +64.3476 8400 CLASS J084013.2705+642053.182 7.00e+00 1.4e+00 0.33 -38362 130.0553 +64.3481

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