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

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Table 5:

Iron K line variability.
Data	Range	Exposure	Counts	$F_{\rm 3-10}$	$I_{\rm FeK}$
	(1)	(2)	(3)	(4)	(5)
Time order
i-1	0-90	40.0	5243	4.0	$\rm 7.5^{+2.3}_{-1.9}$
i-2	90-160	29.8	2450	2.5	$\rm 8.1^{+1.9}_{-2.2}$
i-3	160-230	29.0	4117	4.3	$\rm 7.1^{+3.1}_{-2.1}$
Flux order
L	$\leq$ 0.30	51.8	3592	2.2	$\rm 5.7^{+1.7}_{-1.5}$
M	0.30-0.55	31.7	4772	4.4	$\rm 7.0^{+1.8}_{-2.6}$
H	$\geq$ 0.55	16.2	3681	6.7	$\rm 9.4^{+3.4}_{-3.9}$

Notes. (1) in unit of 10³ s in the light curve in Fig. 1 for the time intervals, or cts^-1for the source count rate range (2) 10³ s (3) background-corrected integrated counts (4) 3-10 keV flux in 10^-12 ergs^-1cm^-2 (5) Fe K line flux in 10^-6 phs^-1cm^-2. Note: the error in the line flux is of the order of $1\sigma$ .

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