Complement to VIII/85A

Source TXS_1129+371: 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 112955+371053 2.35e+03 4.7e+02 252.00 48914 0 -0.86 5.31 173.1492 +36.9053 151 7C 112955.60+371052.00 2.36e+03 4.7e+02 70.20 48914 0 -0.75 4.84 173.1483 +36.9050 178 4C +37.31 2.60e+03 7.8e+02 690.00 48914 0 -0.86 5.31 173.1496 +36.8683 232 MY 112955.6+365423.2 1.54e+03 3.1e+02 150.00 48914 0 -0.86 5.31 173.1488 +36.9064 325 WN B1129.9+3710 1.50e+03 3.0e+02 12.00 48914 0 -0.87 5.26 173.1482 +36.9040 365 TXS 1129+371 1.42e+03 2.8e+02 6.00 48914 0 -0.94 5.52 173.1485 +36.9046 408 B2.3 1129+37 1.20e+03 2.4e+02 0.00 48914 0 -0.88 5.37 173.1513 +36.9033 1400 FIRST J113235.9+365412 2.60e+02 5.2e+01 5.00 48914 0 -0.94 5.52 173.1496 +36.9034 1400 NVSS J113235+365416 4.34e+02 8.7e+01 45.00 48914 0 -0.94 5.52 173.1483 +36.9046 1400 WB 1129+3711 4.16e+02 8.3e+01 120.00 48914 0 -0.86 5.25 173.1546 +36.9097 4850 87GB 112956.9+371107 1.36e+02 2.7e+01 138.00 48914 0 -0.75 4.84 173.1542 +36.9092 4850 BWE 1129+3711 1.13e+02 2.3e+01 138.00 48914 0 -0.87 5.28 173.1546 +36.9097 4850 GB6 B1129+3710 1.17e+02 2.3e+01 108.00 48914 0 -0.86 5.31 173.1529 +36.9053 4850 MITG J113240+3654 1.08e+02 2.2e+01 258.00 48914 0 -0.94 5.52 173.1675 +36.9142

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 J1132.5+3654 2.85e+03 5.7e+02 79.98 -48914 173.1492 +36.9044 151 6C 112955+371053 2.35e+03 4.7e+02 252.00 48914 173.1492 +36.9053 151 7C 112955.60+371052.00 2.36e+03 4.7e+02 70.20 48914 173.1483 +36.9050 178 4C +37.31 2.60e+03 7.8e+02 690.00 48914 173.1496 +36.8683 232 MY 112955.6+365423.2 1.54e+03 3.1e+02 150.00 48914 173.1488 +36.9064 232 MY 112955.9+365521.6 5.10e+02 1.5e+02 150.00 -48914 173.1500 +36.9227 325 WN B1129.9+3710 1.50e+03 3.0e+02 12.00 48914 173.1482 +36.9040 365 TXS 1129+371 1.42e+03 2.8e+02 6.00 48914 173.1485 +36.9046 408 B2.3 1129+37 1.20e+03 2.4e+02 0.00 48914 173.1513 +36.9033 1400 FIRST J113227.7+365234 8.00e-01 2.0e-01 5.00 -48914 173.1155 +36.8763 1400 FIRST J113235.1+365422 1.68e+02 3.4e+01 5.00 -48914 173.1465 +36.9062 1400 FIRST J113235.9+365412 2.60e+02 5.2e+01 5.00 48914 173.1496 +36.9034 1400 WB 1129+3711 4.16e+02 8.3e+01 120.00 48914 173.1546 +36.9097 4850 GB6 B1129+3710 1.17e+02 2.3e+01 108.00 48914 173.1529 +36.9053

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