Complement to VIII/85A

Source VLSS_J1416.0+3558: 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 J1416.0+3558 2.39e+03 4.8e+02 79.98 59438 4 -0.96 5.17 214.0213 +35.9800 151 6C 141358+361251 1.28e+03 2.6e+02 252.00 59438 4 -0.91 5.08 214.0217 +35.9828 151 7C 141358.39+361242.00 1.21e+03 2.4e+02 70.20 59438 4 -0.96 5.17 214.0213 +35.9803 232 MY 141358.6+355853.2 7.20e+02 1.4e+02 150.00 59438 4 -0.98 5.25 214.0221 +35.9814 325 WN B1413.9+3612 6.36e+02 1.3e+02 12.00 59438 4 -0.91 5.07 214.0211 +35.9806 365 TXS 1413+362 5.83e+02 1.2e+02 6.00 59438 4 -0.91 5.08 214.0215 +35.9806 408 B2.3 1413+36 5.63e+02 1.1e+02 0.00 59438 4 -0.99 5.26 214.0175 +35.9900 1400 FIRST J141604.8+355846 1.18e+02 2.4e+01 5.00 59438 4 -0.98 5.25 214.0202 +35.9797 1400 NVSS J141605+355849 1.53e+02 3.1e+01 45.00 59438 4 -0.91 5.08 214.0210 +35.9804 1400 WB 1414+3612 1.43e+02 2.9e+01 120.00 59438 4 -0.91 5.10 214.0312 +35.9703 4850 87GB 141400.5+361206 6.00e+01 1.2e+01 138.00 59438 4 -0.98 5.25 214.0300 +35.9703 4850 BWE 1414+3612 5.70e+01 1.1e+01 138.00 59438 4 -0.98 5.25 214.0312 +35.9703 4850 GB6 B1413+3612 5.30e+01 1.1e+01 108.00 59438 4 -0.98 5.25 214.0271 +35.9736 4850 MITG J141607+3558 5.60e+01 1.1e+01 258.00 59438 4 -0.98 5.25 214.0317 +35.9742

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 J1416.0+3558 2.39e+03 4.8e+02 79.98 59438 214.0213 +35.9800 151 6C 141358+361251 1.28e+03 2.6e+02 252.00 59438 214.0217 +35.9828 151 7C 141358.39+361242.00 1.21e+03 2.4e+02 70.20 59438 214.0213 +35.9803 232 MY 141358.6+355853.2 7.20e+02 1.4e+02 150.00 59438 214.0221 +35.9814 408 B2.3 1413+36 5.63e+02 1.1e+02 0.00 59438 214.0175 +35.9900 1400 FIRST J141604.8+355846 1.18e+02 2.4e+01 5.00 59438 214.0202 +35.9797 1400 FIRST J141605.2+360051 1.40e+00 3.0e-01 5.00 -59438 214.0218 +36.0142 1400 FIRST J141605.9+355859 2.56e+01 5.1e+00 5.00 -59438 214.0249 +35.9831 1400 FIRST J141609.3+355712 1.20e+00 2.0e-01 5.00 -59438 214.0391 +35.9534 1400 FIRST J141615.8+355946 1.40e+00 3.0e-01 5.00 -59438 214.0661 +35.9963 1400 NVSS J141614+355943 2.70e+00 5.0e-01 45.00 -59438 214.0606 +35.9954 4850 GB6 B1413+3612 5.30e+01 1.1e+01 108.00 59438 214.0271 +35.9736 4850 MITG J141607+3558 5.60e+01 1.1e+01 258.00 59438 214.0317 +35.9742

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