Complement to VIII/85A

Source FIRST_J085448.8+200630: 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 J0854.8+2006 6.20e+02 1.2e+02 79.98 34221 0 0.35 2.14 133.7029 +20.1102 365 TXS 0851+202 1.13e+03 2.3e+02 6.00 34221 0 0.34 2.15 133.7037 +20.1086 1400 FIRST J085448.8+200630 1.18e+03 2.4e+02 5.00 34221 0 0.29 2.28 133.7037 +20.1085 1400 NVSS J085448+200630 1.51e+03 3.0e+02 45.00 34221 0 0.29 2.28 133.7036 +20.1085 1400 WB 0851+2017 2.28e+03 4.6e+02 120.00 34221 0 0.38 2.08 133.7046 +20.1053 1465 [P82] 0851+202 1.70e+03 3.4e+02 25.80 34221 0 0.34 2.16 133.7036 +20.1085 2700 PKS J0854+2006 3.42e+03 6.8e+02 60.00 34221 0 0.35 2.14 133.7033 +20.1083 2700 RGB11 J0854.8+2006 1.92e+03 3.8e+02 258.00 34221 0 0.32 2.20 133.7046 +20.1050 4850 87GB 085157.5+201747 2.98e+03 6.0e+02 138.00 34221 0 0.38 2.08 133.7046 +20.1053 4850 BWE 0851+2017 2.62e+03 5.2e+02 138.00 34221 0 0.33 2.17 133.7046 +20.1053 4850 GB6 B0851+2018 3.32e+03 6.6e+02 108.00 34221 0 0.38 2.07 133.7017 +20.1131 4850 IRAS F08519+2017 2.69e+03 5.4e+02 210.00 34221 0 0.39 2.07 133.7050 +20.1089 4850 MITG J085448+2006 3.63e+03 7.3e+02 258.00 34221 0 0.29 2.28 133.7025 +20.1042 4885 [P82a] 0851+202 2.33e+03 4.7e+02 6.00 34221 0 0.35 2.14 133.7036 +20.1085 4885 RGB 0854+201 2.91e+03 5.8e+02 4.02 34221 0 0.35 2.14 133.7036 +20.1085 8400 CLASS J085448.8740+200630.638A 3.00e+03 6.0e+02 0.33 34221 0 0.33 2.17 133.7036 +20.1085 8400 CLASS J085448.8740+200630.638B 3.83e+03 7.7e+02 0.33 34221 0 0.35 2.14 133.7036 +20.1085 8400 JVAS J0854+2006 3.70e+03 7.4e+02 0.33 34221 0 0.35 2.14 133.7036 +20.1085 10700 RGB2 J0854.8+2006 2.74e+03 5.5e+02 72.00 34221 0 0.36 2.03 133.7046 +20.1050

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 J0854.8+2006 6.20e+02 1.2e+02 79.98 34221 133.7029 +20.1102 1400 FIRST J085447.1+200644 1.50e+00 3.0e-01 5.00 -34221 133.6966 +20.1123 1400 FIRST J085447.6+200629 1.00e+00 2.0e-01 5.00 -34221 133.6987 +20.1081 1400 FIRST J085453.4+200623 1.60e+00 3.0e-01 5.00 -34221 133.7228 +20.1065 2700 PKS J0854+2006 3.42e+03 6.8e+02 60.00 34221 133.7033 +20.1083 2700 RGB11 J0854.8+2006 1.92e+03 3.8e+02 258.00 34221 133.7046 +20.1050 4850 IRAS F08519+2017 2.69e+03 5.4e+02 210.00 34221 133.7050 +20.1089 4850 MITG J085448+2006 3.63e+03 7.3e+02 258.00 34221 133.7025 +20.1042

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