Complement to VIII/85A

Source 4C_+01.66: 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 J2135.8+0118 3.84e+03 7.7e+02 79.98 88277 0 -0.60 4.80 323.9692 +01.3048 80 Cula 2133+010 3.00e+03 6.0e+02 222.00 88277 0 -0.59 4.77 323.9717 +01.3011 160 Culb 2133+010 3.00e+03 6.0e+02 111.00 88277 0 -0.54 4.60 323.9717 +01.3011 178 4C +01.66 2.40e+03 7.2e+02 690.00 88277 0 -0.60 4.80 323.9617 +01.2650 365 TXS 2133+010 2.16e+03 4.3e+02 6.00 88277 0 -0.60 4.80 323.9686 +01.3045 408 MRC 2133+010 1.81e+03 3.6e+02 120.00 88277 0 -0.60 4.80 323.9700 +01.3064 1400 FIRST J213552.5+011815 8.46e+02 1.7e+02 5.00 88277 0 -0.60 4.80 323.9688 +01.3044 1400 NVSS J213552+011815 8.33e+02 1.7e+02 45.00 88277 0 -0.60 4.80 323.9687 +01.3044 1400 WB 2133+0104 8.18e+02 1.6e+02 120.00 88277 0 -0.60 4.80 323.9679 +01.3031 2700 PKS J2135+0118 5.50e+02 1.1e+02 60.00 88277 0 -0.60 4.80 323.9688 +01.3042 4850 87GB 213319.3+010446 3.93e+02 7.9e+01 138.00 88277 0 -0.59 4.77 323.9679 +01.3036 4850 BWE 2133+0104 2.93e+02 5.9e+01 138.00 88277 0 -0.75 5.23 323.9679 +01.3031 4850 GB6 B2133+0104 4.08e+02 8.2e+01 108.00 88277 0 -0.56 4.67 323.9650 +01.3058 4850 MITG J213553+0117 3.17e+02 6.3e+01 258.00 88277 0 -0.60 4.80 323.9733 +01.3000 4850 PMN J2135+0118 3.65e+02 7.3e+01 168.00 88277 0 -0.60 4.80 323.9683 +01.3058

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
178 4C +01.66 2.40e+03 7.2e+02 690.00 88277 323.9617 +01.2650 1400 FIRST J213538.0+011743 1.50e+00 3.0e-01 5.00 -88277 323.9083 +01.2953 1400 FIRST J213543.8+011502 1.54e+01 3.1e+00 5.00 -88277 323.9329 +01.2508 1400 FIRST J213545.0+011923 9.00e-01 2.0e-01 5.00 -88277 323.9376 +01.3232 1400 FIRST J213552.6+012055 7.00e-01 2.0e-01 5.00 -88277 323.9692 +01.3488 1400 FIRST J213554.6+012017 1.00e+00 2.0e-01 5.00 -88277 323.9778 +01.3381 1400 FIRST J213559.2+011841 7.00e-01 2.0e-01 5.00 -88277 323.9967 +01.3115 1400 FIRST J213559.9+011740 9.00e-01 2.0e-01 5.00 -88277 324.0000 +01.2945 1400 NVSS J213543+011502 1.49e+01 3.0e+00 45.00 -88277 323.9329 +01.2506 4850 87GB 213319.3+010446 3.93e+02 7.9e+01 138.00 88277 323.9679 +01.3036 4850 MITG J213553+0117 3.17e+02 6.3e+01 258.00 88277 323.9733 +01.3000 4850 PMN J2135+0118 3.65e+02 7.3e+01 168.00 88277 323.9683 +01.3058

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