Complement to VIII/85A

Source MRC_1601+173: 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 J1603.5+1711 1.79e+03 3.6e+02 79.98 67746 5 -0.39 3.99 240.8829 +17.1998 80 Cula 1601+173 3.00e+03 6.0e+02 222.00 67746 5 -0.39 3.99 240.8770 +17.1889 160 Culb 1601+173 1.60e+03 3.2e+02 111.00 67746 5 -0.57 4.57 240.8770 +17.1889 408 MRC 1601+173 1.26e+03 2.5e+02 120.00 67746 5 -0.39 3.99 240.8800 +17.1961 1400 NVSS J160332+171158 4.56e+02 9.1e+01 45.00 67746 5 -0.44 4.07 240.8839 +17.1997 1400 WB 1601+1719 6.86e+02 1.4e+02 120.00 67746 5 -0.43 4.16 240.8825 +17.1942 2700 PKS J1603+1711 4.70e+02 9.4e+01 60.00 67746 5 -0.39 3.99 240.8817 +17.1933 4850 87GB 160115.8+171951 4.11e+02 8.2e+01 138.00 67746 5 -0.40 4.08 240.8812 +17.1942 4850 BWE 1601+1719 3.36e+02 6.7e+01 138.00 67746 5 -0.40 4.00 240.8825 +17.1942 4850 GB6 B1601+1720 3.94e+02 7.9e+01 108.00 67746 5 -0.39 3.99 240.8829 +17.1992 4850 MITG J160330+1711 2.86e+02 5.7e+01 258.00 67746 5 -0.44 4.07 240.8775 +17.1953 4850 MITG J160331+1711 3.45e+02 6.9e+01 258.00 67746 5 -0.44 4.07 240.8808 +17.1872

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 J1603.5+1711 1.79e+03 3.6e+02 79.98 67746 240.8829 +17.1998 160 Culb 1601+173 1.60e+03 3.2e+02 111.00 67746 240.8770 +17.1889 365 TXS 1601+173 7.26e+02 1.5e+02 6.00 -67746 240.8841 +17.1994 408 MRC 1601+173 1.26e+03 2.5e+02 120.00 67746 240.8800 +17.1961 1400 FIRST J160330.1+170959 1.10e+00 2.0e-01 5.00 -67746 240.8757 +17.1665 1400 FIRST J160332.1+171156 2.95e+02 5.9e+01 5.00 -67746 240.8838 +17.1992 1400 FIRST J160332.9+171246 4.30e+00 9.0e-01 5.00 -67746 240.8872 +17.2129 1400 NVSS J160326+171000 1.60e+02 3.2e+01 45.00 -67746 240.8587 +17.1668 1400 NVSS J160332+171158 4.56e+02 9.1e+01 45.00 67746 240.8839 +17.1997 1400 NVSS J160332+171303 1.53e+01 3.1e+00 45.00 -67746 240.8850 +17.2177 1400 WB 1601+1719 6.86e+02 1.4e+02 120.00 67746 240.8825 +17.1942 2700 PKS J1603+1711 4.70e+02 9.4e+01 60.00 67746 240.8817 +17.1933 4850 MITG J160330+1711 2.86e+02 5.7e+01 258.00 67746 240.8775 +17.1953 4850 MITG J160331+1711 3.45e+02 6.9e+01 258.00 67746 240.8808 +17.1872 8400 CLASS J160332.0842+171155.326 4.67e+01 9.3e+00 0.33 -67746 240.8837 +17.1987 8400 JVAS J1603+1711 5.40e+01 1.1e+01 0.33 -67746 240.8837 +17.1987

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