**Table 1:** The log of all the analyzed observations. The reported fluxes are relative to the fits shown in Table 2.
Object	Date	EPIC-pn		PDS	PDS/pn	z	${N_{\rm Hg}}^{c}$	${F}_{\rm 2-10~keV}$	${\rm log}~{L_{\rm 2-10~keV}}^{d}$
		Mode^a	T^b (ks)	T (ks)	factor		10²⁰ cm^-2	$\times10^{-11}$ (cgs)
ESO198-G024	2001-01-23/26	M/F	16	63	0.99	0.045500	3.09	1.3	43.77
MCG-02-58-022	2000-12-01/05	T/S	7	47	0.92	0.047316	3.60	3.1	44.18
NGC 7213	2001-05-27/30	T/S	30	38	0.89	0.005977	2.04	2.2	42.24
NGC 5548	2001-07-08/12	T/S	49	48	0.91	0.017175	1.69	4.0	43.41
MKN 841	2001-01-11/14	T/S	16	41	0.90	0.036422	2.34	1.6	43.67
IC 4329A	2001-01-31/02-01	M/F	10	16	1.01	0.016054	4.42	3.7	43.39
NGC 3516	2001-04-10/12	T/S	57	40	1.08	0.00884	3.05	2.4	42.69
NGC 5506	2001-02-01/03	M/L	14	38	1.16	0.006181	3.81	7.8	42.95

^a Filter/Frame: M = Medium, T = Thin, F = Full Frame, L = Large Window, S = Small Window.
^b After screening for intervals of flaring particle background (see text for details).
^c Values from Dickey & Lockman (1990).
^d Log of luminosity corrected for absorption (see Table 2) in erg s^-1 (H₀=70 km s^-1 Mpc^-1).

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