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Home All issues Volume 498 / No 1 (April IV 2009) A&A, 498 1 (2009) 61-66 Full HTML
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Table 3:

XMM-Newton EPIC best-fit parameters.
$\Gamma$ $\rm 1.69^{+0.18}_{-0.10}$
R $\rm 2.7^{+0.81}_{-0.60}$
$N_{\rm G}$ ( $3.06\times10^{20}$) cm-2
$N_{\rm H}$ $(7.14^{+1.75}_{-1.21}) \times10^{23}$ cm-2
n $(1.83^{+0.47}_{-0.31}) \times10^{-3}$
$n_{\rm unobscured}$ $(8.1^{+4.08}_{-7.28}) \times10^{-6}$
$E_{\rm Fe~~}$ (keV) $\rm 6.40^{+0.13}_{-0.08}$
$F_{\rm Fe~~}$ $(3.65^{+3.93}_{-2.04})\times10^{-5}$
EW (eV) $\rm 206^{+199}_{-115}$
$\chi^{2}$(d.o.f.) 37.5(37)
Unabsorbed luminosity and absorbed flux
$L_{2-10~{\rm keV}}$ (erg s-1) $7.53 \times10^{43}$
$\rm Flux_{2-10~keV}$ (erg s-1 cm-2) $2.64 \times 10^{-12}$
Normalizations n are expressed in cm-2 s-1 keV-1; the normalization
of the iron line is expressed in photons cm-2 s-1.

Source LaTeX | All tables | In the text

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