Complement to VIII/85A

Source FIRST_J075738.0+252812: 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
365 TXS 0754+256 2.14e+02 4.3e+01 6.00 32208 0 -0.23 2.93 119.4099 +25.4692 1400 FIRST J075738.0+252812 1.63e+02 3.3e+01 5.00 32208 0 -0.36 3.39 119.4086 +25.4702 1400 NVSS J075738+252812 1.57e+02 3.1e+01 45.00 32208 0 -0.32 3.26 119.4087 +25.4702 1400 WB 0754+2536 1.45e+02 2.9e+01 120.00 32208 0 -0.32 3.26 119.4129 +25.4719 4850 87GB 075437.1+253625 1.63e+02 3.3e+01 138.00 32208 0 -0.32 3.26 119.4117 +25.4719 4850 GB6 B0754+2536 1.51e+02 3.0e+01 108.00 32208 0 -0.32 3.26 119.4104 +25.4706 4850 MITG J075734+2528 1.12e+02 2.2e+01 258.00 32208 0 -0.32 3.26 119.3954 +25.4750 8400 CLASS J075738.0754+252812.746 9.73e+01 1.9e+01 0.33 32208 0 -0.29 3.12 119.4086 +25.4702
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
No object found

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