The MBH − Mstar relation of obscured AGNs at high redshift

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Table 1

Properties of the X-ray selected obscured AGN with broad Hα.

ID	z	Instr.	log L_{2 − 10 keV}^a	log N_H	log L_bol^b	FWHM_Hα^c	log M_BH	L/L_Edd	log M_star
			[erg s^-1]	[cm^-2]	[erg s^-1]	[km s^-1]	[M_⊙]		[M_⊙]

Ab2690#29	2.087	ISAAC	44.95	22.80	46.81	5871 ± 245	9.44 ± 0.31	0.12	12.50 ± 0.20
XMMES1_460	1.748	SINFONI	44.86	22.50	46.59	2316 ± 113	8.54 ± 0.31	0.63	11.53 ± 0.20
BPM1627#181	1.335	SINFONI	44.20	22.81	45.76	2491 ± 511	8.15 ± 0.36	0.32	11.28 ± 0.20

Notes.

^(a)

Absorption corrected 2–10 keV luminosity.

^(b)

Bolometric luminosity inferred by using the X-ray bolometric corrections given in Marconi et al. (2004).

^(c)

Full Width at Half Maximum of the broad component of Hα in km s^-1.

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