The Suzaku broadband X-ray spectrum of the dwarf Seyfert galaxy NGC 4395

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Table 1:

Spectral fit to the Suzaku XIS time-averaged spectrum.
Data	$\Gamma$	$N_{\rm H}$	$N_{\rm H,W}$	$\xi$	$E_{\rm FeK}$	$\sigma$	$I_{\rm FeK}$	$\chi^2$ /d.o.f.
		cm^-2	cm^-2	ergs^-1cm	keV	keV	phs^-1cm^-2
Total	$\rm 1.40^{+0.05}_{-0.04}$	$5.4^{+2.8}_{-3.0}\times 10^{20}$	$2.1^{+0.3}_{-0.2}\times 10^{22}$	$\rm 34^{+5}_{-4}$	$\rm 6.36^{+0.04}_{-0.04}$	$\rm0.09^{+0.05}_{-0.05}$	$6.4^{+2.2}_{-1.8}\times 10^{-6}$	406.0/407

Notes. The spectrum was obtained by combining the XIS0 and XIS3 data. The model consists of a power law with a Gaussian for the Fe K $\alpha$ line, modified by warm and cold absorption. The cold absorption column is denoted by $N_{\rm H}$ , which is in excess of the Galactic column of $1.85\times 10^{20}$ cm^-2. Tim Kallman's XSTAR grid tables (``grid 25'') with the turbulent velocity of 200 km s^-1 is adopted for the warm absorber modelling.

Source LaTeX | All tables | In the text

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