Complement to VIII/85A

Source NVSS_J074836+240024: 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 J0748.6+2400 3.13e+03 6.3e+02 79.98 31893 0 -0.20 3.80 117.1513 +24.0062 365 TXS 0745+241 1.13e+03 2.3e+02 6.00 31893 0 0.04 2.94 117.1506 +24.0065 408 B2.2 0745+24 1.32e+03 2.6e+02 0.00 31893 0 0.04 2.94 117.1538 +24.0000 408 B2.4 0745+24 1.28e+03 2.6e+02 0.00 31893 0 0.01 3.03 117.1529 +24.0083 1400 FIRST J074836.1+240024 8.62e+02 1.7e+02 5.00 31893 0 0.05 2.86 117.1505 +24.0067 1400 NVSS J074836+240024 9.58e+02 1.9e+02 45.00 31893 0 0.04 2.94 117.1504 +24.0067 1400 WB 0745+2407 9.86e+02 2.0e+02 120.00 31893 0 0.02 3.00 117.1508 +24.0036 2700 RGB11 J0748.6+2400 1.15e+03 2.3e+02 258.00 31893 0 0.01 3.03 117.1504 +24.0036 4850 87GB 074535.6+240745 1.35e+03 2.7e+02 138.00 31893 0 0.01 3.03 117.1500 +24.0039 4850 BWE 0745+2407 1.19e+03 2.4e+02 138.00 31893 0 0.01 3.03 117.1508 +24.0036 4850 GB6 B0745+2407 1.26e+03 2.5e+02 108.00 31893 0 0.01 3.03 117.1500 +24.0058 4850 MITG J074835+2400 1.43e+03 2.9e+02 258.00 31893 0 0.01 3.03 117.1492 +24.0006 4885 [P82a] 0745+241 1.08e+03 2.2e+02 6.00 31893 0 0.04 2.94 117.1504 +24.0067 4885 RGB 0748+240 1.26e+03 2.5e+02 4.02 31893 0 0.04 2.94 117.1505 +24.0067 8400 CLASS J074836.1097+240024.149 1.54e+03 3.1e+02 0.33 31893 0 0.04 2.94 117.1504 +24.0067 8400 JVAS J0748+2400 1.54e+03 3.1e+02 0.33 31893 0 0.01 3.03 117.1505 +24.0067 10700 RGB2 J0748.6+2400 1.11e+03 2.2e+02 72.00 31893 0 0.01 3.03 117.1504 +24.0036

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 J0748.6+2400 3.13e+03 6.3e+02 79.98 31893 117.1513 +24.0062 365 TXS 0745+241 1.13e+03 2.3e+02 6.00 31893 117.1506 +24.0065 408 B2.2 0745+24 1.32e+03 2.6e+02 0.00 31893 117.1538 +24.0000 1400 FIRST J074836.1+240024 8.62e+02 1.7e+02 5.00 31893 117.1505 +24.0067 1400 NVSS J074836+240024 9.58e+02 1.9e+02 45.00 31893 117.1504 +24.0067 2700 PKS J0748+2400 7.40e+02 1.5e+02 60.00 -31893 117.1504 +24.0067 4850 GB6 B0745+2407 1.26e+03 2.5e+02 108.00 31893 117.1500 +24.0058 4850 MITG J074835+2400 1.43e+03 2.9e+02 258.00 31893 117.1492 +24.0006 4885 [P82a] 0745+241 1.08e+03 2.2e+02 6.00 31893 117.1504 +24.0067 8400 CLASS J074836.1097+240024.149 1.54e+03 3.1e+02 0.33 31893 117.1504 +24.0067

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