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Table 1

The GREDOS sample.

Obs.# NED name Typea z fBATb Esoftc red Cte Texpf

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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