On the driver of relativistic effect strength in Seyfert galaxies

M. Guainazzi; S. Bianchi; I. de la Calle Pérez; M. Dovčiak; A. L. Longinotti

doi:10.1051/0004-6361/201016245

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Volume 531 (July 2011)

A&A, 531 (2011) A131

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Table 1

The GREDOS sample.

Obs.#	NED name	Type^a	z	f_BAT^b	E_soft^c	r_e^d	C_t^e	T_exp^f

0006220201	NGC 4507	Sy2	0.012	146.0	3.0	60/67	0.35/0.5	42.0/33.2
0067540201	Mrk 348	Sy2	0.015	112.0	2.5	60/40	1/ 2	26.4/22.5
0110930701	NGC 4388	Sy2	0.008	203.0	3.0	68/32	0.5/ 1	11.5/ 7.3
0144230101	Mrk 6	Sy1.5	0.019	43.7	1.0	85/37	0.35/0.5	36.0/31.3
0145670101	NGC 2110	Sy2	0.008	215.0	1.5	81/35	0.35/0.5	34.0/34.8
0152940101	NGC 5252	Sy2	0.022	60.1	2.0	67/38	0.35/0.35	41.0/33.3
0202860101	NGC 7172	Sy2	0.009	119.0	1.5	77/38	1/ 2	44.6/40.0
0550450301	1ES0241+622	Sy1.2	0.045	51.0	1.0	70/40	1/35	15.2/12.1
0550451501	GRS 1734-292	Sy1	0.021	103.0	1.0	112/38	1/0.5	17.2/13.5
Table 2	NGC 5506	Sy2	0.006	196.0	2.0	50/50	0.35/0.35	61.0/117.8
Table 2	NGC 4151	Sy1.5	0.003	376.0	2.2	38/39	0.35/0.5	87.5/71.9
Table 2	NGC 526A	Sy1.9	0.019	42.6	1.2	89/38	0.35/0.5	53.7/45.4
Table 2	MCG-05-23-016	Sy2	0.008	166.0	1.8	40/47	0.35/0.5	118.4/104.8

Notes.

^(a)

Optical Seyfert type according to the Véron-Cetty & Véron catalogue (Véron-Cetty & Véron 2010).

^(b)

The 14–195 keV BAT flux (in units of 10^-12 erg cm^-2 s^-1) after Cusumano et al. (2010).

^(c)

Low boundary of the energy interval where the spectral fit was performed.

^(d)

Size (in arc-seconds) of the source spectrum extraction region (MOS/pn).

^(e)

Threshold (in counts per second) on the single-event, high-energy light curves to reject intervals of high particle background (MOS/pn).

^(f)

Net exposure time in ks (MOS/pn) after data screening.

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