Complement to VIII/85A

Source CLASS_J131004.4333+340309.087: 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
232 MY 130742.6+340241.4 2.60e+02 5.2e+01 150.00 57333 0 0.29 1.72 197.5121 +34.0448 325 WN B1307.7+3419 3.35e+02 6.7e+01 12.00 57333 0 -0.42 3.68 197.5185 +34.0529 408 5C12 305 4.29e+02 1.2e+02 90.00 57333 0 -0.42 3.68 197.5191 +34.0519 408 5C12a 305 3.64e+02 7.3e+01 79.98 57333 0 -0.42 3.68 197.5187 +34.0527 408 B2.3 1307+34B 3.79e+02 7.6e+01 0.00 57333 0 -0.42 3.68 197.5163 +34.0450 1400 FIRST J131004.4+340309 4.40e+02 8.8e+01 5.00 57333 0 0.19 2.05 197.5184 +34.0525 1400 NVSS J131004+340309 4.32e+02 8.6e+01 45.00 57333 0 0.19 2.05 197.5186 +34.0525 4850 87GB 130743.2+341853 1.90e+02 3.8e+01 138.00 57333 0 -0.42 3.68 197.5146 +34.0489 4850 GB6 B1307+3418 1.69e+02 3.4e+01 108.00 57333 0 -0.42 3.68 197.5129 +34.0506 4850 MITG J131006+3403 1.74e+02 3.5e+01 258.00 57333 0 -0.42 3.68 197.5275 +34.0503 8400 CLASS J131004.4333+340309.087 8.99e+01 1.8e+01 0.33 57333 0 -0.42 3.68 197.5185 +34.0525 8400 CLASS J131004.4333+340309.115 1.06e+02 2.1e+01 0.33 57333 0 -0.42 3.68 197.5185 +34.0525

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 7C 130744.39+341913.00 1.56e+02 3.1e+01 70.20 -57333 197.5196 +34.0544 232 MY 130742.6+340241.4 2.60e+02 5.2e+01 150.00 57333 197.5121 +34.0448 325 WN B1307.7+3419 3.35e+02 6.7e+01 12.00 57333 197.5185 +34.0529 408 5C12 305 4.29e+02 1.2e+02 90.00 57333 197.5191 +34.0519 408 B2.3 1307+34B 3.79e+02 7.6e+01 0.00 57333 197.5163 +34.0450 1400 FIRST J131004.4+340309 4.40e+02 8.8e+01 5.00 57333 197.5184 +34.0525 1400 NVSS J131004+340309 4.32e+02 8.6e+01 45.00 57333 197.5186 +34.0525 1400 WB 1307+3418 5.52e+02 1.1e+02 120.00 -57333 197.5163 +34.0506 4850 BWE 1307+3418 1.48e+02 3.0e+01 138.00 -57333 197.5163 +34.0506 4850 GB6 B1307+3418 1.69e+02 3.4e+01 108.00 57333 197.5129 +34.0506 8400 CLASS J131002.6379+340256.494 1.50e+00 3.0e-01 0.33 -57333 197.5110 +34.0490 8400 CLASS J131003.4961+340303.966 1.70e+00 3.0e-01 0.33 -57333 197.5145 +34.0511 8400 CLASS J131004.4333+340309.087 8.99e+01 1.8e+01 0.33 57333 197.5185 +34.0525 8400 CLASS J131005.3776+340314.266 1.20e+00 2.0e-01 0.33 -57333 197.5224 +34.0540 8400 CLASS J131006.0744+340302.029 1.70e+00 3.0e-01 0.33 -57333 197.5253 +34.0506

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