HESS J1632-478: an energetic relic | Astronomy & Astrophysics (A&A)

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Table 3:

Best fit parameters for an absorbed power-law model fitted simultaneously to the three EPIC spectra on the point-like and extended sources.
Parameter	Point	Extended	Unit
$N_{\rm H}$	$\rm 13_{-4}^{+6}$	$\rm 11_{-2.7}^{+2.2}$	10²² cm^-2
$\Gamma$	$\rm 2.6_{-0.8}^{+1.3}$	$\rm 3.4_{-0.8}^{+0.6}$
$F_{\rm 2{-}10~keV}$	$\rm 2.3_{-1.0}^{+0.3}$	$\rm 4.3 _{-0.4}^{+0.8}$	$\rm 10^{-13}$ erg cm^-2 s^-1
$\chi^2_\nu$	1.8	1.9

Notes. Reported errors correspond to $1\sigma$ uncertainties (68%). The 2-10 keV fluxes are corrected for the absorption.

Source LaTeX | All tables | In the text

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