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Home All issues Volume 508 / No 3 (December IV 2009) A&A, 508 3 (2009) 1275-1278 Full HTML
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Table 1:

Best fit parameters obtained from modeling the joint XIS and HXD data in the 5-60 keV band.
$A_{{\rm cutoffpl}}=3.79_{-0.03}^{+0.05}\times 10^{-2}$ $F_{{\rm Fe\ K}\alpha_1}=3.7\pm0.1\times 10^{-3}$ $F_{{\rm Fe\ K}\alpha_2}=1.85\pm0.05\times 10^{-3}$  
  $F_{{\rm Fe\ K}\beta_1}=3.2_{-0.4}^{+0.3}\times 10^{-4}$ $F_{{\rm Fe\ K}\beta_3}=1.57_{-0.20}^{+0.15}\times 10^{-4}$ $F_{{\rm Ni\ K}\alpha}=7.4_{-2.7}^{+2.2}\times 10^{-4}$
$c=1.00\pm0.01$ $\Gamma=0.676_{-0.042}^{+0.009}$ $E_{\rm Fold} =20.5_{-0.3}^{+0.6}$ keV  
$N_{\rm H}=1.95_{-0.03}^{+0.02} \times 10^{24}~{\rm cm}^{-2}$ $A_{\rm Fe} =1.14_{-0.02}^{+0.03}$    
$E_{{\rm Fe\ K}\alpha_1}=6404_{-2}^{+3}$ eV ${\it EW}_{{\rm Fe\ K}\alpha_1}=467_{-54}^{+13}$ eV $E_{{\rm Fe\ K}\alpha_2}=6391_{-2}^{+3}$ eV ${\it EW}_{{\rm Fe\ K}\alpha_2}=233_{-27}^{+7}$ eV
$E_{{\rm Fe\ K}\beta_1}=7093_{-14}^{+13}$ eV ${\it EW}_{{\rm Fe\ K}\beta_1}=44.1_{-5.2}^{+1.4}$ eV $E_{{\rm Fe\ K}\beta_3}=7092_{-14}^{+13}$ eV ${\it EW}_{{\rm Fe\ K}\beta_3}=22.1_{-2.7}^{+0.6}$ eV
$E_{{\rm Ni\ K}\alpha}=7446_{-51}^{+46}$ eV ${\it EW}_{{\rm Ni\ K}\alpha}=108_{-12.7}^{+4}$ eV    
$F_{5.0-60~{\rm keV}}^{\rm ~absorbed}=3.4_{-0.1}^{+0.7}~10^{-10}~{\rm erg}~{\rm cm}^{-2}~{\rm s}^{-1}$ $F_{5.0-60~{\rm keV}}^{\rm ~unabsorbed}=2.43_{-0.09}^{+0.44}~10^{-9}~{\rm erg}~{\rm cm}^{-2}~{\rm s}^{-1}$ $\chi^{2}/{\rm d.o.f.}=242.6/245$ $\chi^2_{\rm red}=0.99$

We list the photon index ($\Gamma$), folding energy ( $E_{\rm Fold}$), hydrogen equivalent column ($N_{\rm H}$), Fe abundance ( $A_{\rm Fe}$), the total absorbed and unabsorbed fluxes, and the energy (E) and equivalent width (${\it EW}$) of the fluorescence lines. The norm of the absorbed cutoff powerlaw ( $A_{{\rm cutoffpl}}$) is defined as the photon flux at 1 keV; for the absorbed Gaussian lines the norm (F) equals the total line flux.

Source LaTeX | All tables | In the text

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