**Table 1:** The sample.
PG name	Other name	RA	Dec	z	$N^{\rm Gal}_{\rm H}$
		(J2000)	(J2000)		(10 $^{20}~{\rm cm^{-2}}$ )
0007+106 $^\star$	III Zw 2	00 10 31.0	+10 58 30	0.089	6.09^a
0050+124	I Zw 1	00 53 34.9	+12 41 36	0.061	4.99^a
0157+001	MKN 1014	01 59 50.2	+00 23 41	0.163	2.46^b
0804+761	1H 0758+762	08 10 58.6	+76 02 42	0.100	3.26^c
0844+349	TON 914	08 47 42.4	+34 45 04	0.064	3.32^c
0947+396^L		09 50 48.4	+39 26 50	0.206	1.92^b
0953+414^L		09 56 52.1	+41 15 34	0.239	1.12^c
1001+054^L		10 04 20.1	+05 13 00	0.161	1.88^a
1048+342^L		10 51 43.8	+33 59 26	0.167	1.75^b
1100+772 $^\star$	3C 249.1	11 04 13.7	+76 58 58	0.312	3.17^e
1114+445^L		11 17 06.4	+44 13 33	0.144	1.93^b
1115+080		11 18 16.0	+07 45 59	1.718	3.62^b
1115+407^L		11 18 30.2	+40 25 53	0.154	1.74^b
1116+215^L	TON 1388	11 19 08.6	+21 19 18	0.177	1.44^a
1202+281^L		12 04 42.1	+27 54 11	0.165	1.72^d
1206+459		12 08 58.0	+45 40 35	1.158	1.31^d
1211+143		12 14 17.7	+14 03 13	0.081	2.76^c
1216+069^L		12 19 20.9	+06 38 38	0.334	1.57^c
1226+023 $^{L\star}$	3C 273	12 29 06.7	+02 03 08	0.158	1.89^d
1244+026		12 46 35.3	+02 22 09	0.048	1.93^a
1307+085		13 09 47.0	+08 19 48	0.155	2.11^d
1309+355 $^{L\star}$	TON 1565	13 12 17.8	+35 15 21	0.184	1.00^b
1322+659^L		13 23 49.5	+65 41 48	0.168	1.89^b
1352+183^L		13 54 35.6	+18 05 17	0.158	1.84^a
1402+261^L		14 05 16.2	+25 55 35	0.164	1.42^a
1404+226		14 06 21.8	+22 23 35	0.095	3.22^a
1407+265		14 07 07.8	+26 32 30	0.940	1.38^a
1411+442^L		14 13 48.3	+44 00 14	0.0896	1.05^c
1415+451^L		14 17 01.24	+44 56 16	0.114	1.10^e
1427+480^L		14 29 43.0	+47 47 26	0.221	1.69^b
1440+356^L	MKN 478	14 42 07.4	+35 26 23	0.079	0.97^b
1444+407^L		14 46 45.9	+40 35 05	0.267	1.27^e
1501+106	MKN 841	15 04 01.2	+10 26 16	0.036	2.19^b
1512+370 $^{L\star}$	4C +37.43	15 14 43.0	+36 50 50	0.371	1.36^e
1613+658	MKN 876	16 13 57.2	+65 43 09	0.129	2.66^a
1626+554^L		16 27 56.0	+55 22 31	0.133	1.55^b
1630+377		16 32 01.2	+37 37 49	1.466	0.90^a
1634+706		16 34 31.4	+70 31 34	1.334	5.74^a
2214+139	MKN 304	22 17 11.5	+14 14 28	0.066	4.96^d
2302+029		23 04 45.0	+03 11 46	1.044	5.27^d

$^\star$ Radio-loud objects. ^L Objects included in Laor et al. (1997). References for $N_{\rm H}$ values: ^a Elvis et al. (1989); ^b Murphy et al. (1996); ^c Lockman & Savage (1995); ^d Dickney & Lockman (1990); ^e Stark et al. (1992).

Source LaTeX | All tables | In the text

	1 Introduction
	2 XMM-Newton observations
	3 Analysis of the spectra
	4 Discussion
	5 Conclusions
	References
	Online Material