Unveiling the nature of INTEGRAL objects through optical spectroscopy - VIII. Identification of 44 newly detected hard X-ray sources

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Volume 519 (September 2010)

A&A, 519 (2010) A96

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Table 4:

Synoptic table containing the main results concerning the 18 broad emission-line AGNs (Figs. 8-10) identified or observed in the present sample of *INTEGRAL* sources.
Object	$F_{\rm H_\alpha}$	$F_{\rm H_\beta}$	$F_{\rm [OIII]}$	Class	z	D_L (Mpc)	$E(B-V)_{\rm Gal}$	$L_{\rm X}$
IGR J00158+5605	^*	27.7 $\pm$ 1.3	30.0 $\pm$ 0.9	Sy1.5	0.169	875.5	0.427	1.8 (0.1-2.4)
	^*	[88 $\pm$ 4]	[94 $\pm$ 3]					6.1 (0.2-2)
								35 (20-40)
								<26 (40-100)
IGR J02086-1742	^*	120 $\pm$ 12	38.5 $\pm$ 1.9	Sy1.2	0.129	651.8	0.028	1.1 (0.1-2.4)
	^*	[126 $\pm$ 13]	[42 $\pm$ 2]					33 (2-10)
								140 (20-100)
IGR J06058-2755	^*	58 $\pm$ 6	66 $\pm$ 3	Sy1.5	0.090	443.1	0.030	5.0 (0.1-2.4)
	^*	[64 $\pm$ 6]	[72 $\pm$ 4]					30 (0.2-12)
								36 (17-60)
Swift J0845.0-3531	^*	26.3 $\pm$ 1.3	5.4 $\pm$ 0.3	Sy1.2	0.137	695.7	0.531	5.9 (0.1-2.4)
	^*	[112 $\pm$ 6]	[22.9 $\pm$ 1.6]					78 (14-150)
								50 (17-60)
IGR J09094+2735	^*	4.7 $\pm$ 0.3	1.36 $\pm$ 0.04	NLSy1	0.2844	1572.4	0.030	6.7 (0.1-2.4)
	^*	[4.8 $\pm$ 0.3]	[1.51 $\pm$ 0.05]					920 (17-60)
PKS 1143-696	^*	48 $\pm$ 2	1.0 $\pm$ 0.1	Sy1.2	0.244	1320.2	0.385	23 (0.1-2.4)
	^*	[134 $\pm$ 7]	[2.4 $\pm$ 0.2]					120 (2-10)
								230 (17-60)
								280 (20-100)
IGR J12107+3822	^*	109 $\pm$ 7	64.2 $\pm$ 1.9	Sy1.5	0.0229	107.5	0.021	0.31 (0.2-12)
	^*	[115 $\pm$ 7]	[68 $\pm$ 2]					1.8 (14-150)
								1.6 (17-60)
IGR J1248.2-5828	^*	1.1 $\pm$ 0.3	7.8 $\pm$ 0.5	Sy1.9	0.028	131.9	0.624	0.85 (2-10)
	^*	[5.8 $\pm$ 1.6]	[54 $\pm$ 4]					1.6 (17-60)
								2.1 (20-100)
IGR J13168-7157	^*	67 $\pm$ 10	47.1 $\pm$ 1.4	Sy1.5	0.070	339.9	0.255	0.60 (0.1-2.4)
	^*	[160 $\pm$ 20]	[103 $\pm$ 3]					11 (0.2-12)
								13 (17-60)
IGR J13187+0322	--	17.2 $\pm$ 1.7	1.5 $\pm$ 0.3	Type 1	0.6058	3846.2	0.031	<540 (20-40)
	--	[17.2 $\pm$ 1.7]	[1.5 $\pm$ 0.3]	QSO				<1300 (40-100)
Swift J1513.8-8125	^*	103 $\pm$ 5	37.3 $\pm$ 1.1	Sy1.2	0.069	334.8	0.272	20 (14-150)
	^*	[223 $\pm$ 11]	[83 $\pm$ 2]					34 (14-195)
								15 (17-60)
IGR J15311-3737	--	48 $\pm$ 2	6.9 $\pm$ 0.3	Sy1	0.127	640.8	0.320	2.3 (0.1-2.4)
	--	[120 $\pm$ 4]	[16.6 $\pm$ 0.5]					12-16 (0.2-12)
								44 (20-100)
IGR J18078+1123	^*	64 $\pm$ 4	12.6 $\pm$ 0.6	Sy1/1.2	0.078	380.9	0.131	1.2 (0.1-2.4)
	^*	[90 $\pm$ 6]	[18.6 $\pm$ 0.9]					51 (17-60)
IGR J19077-3925	^*	4.8 $\pm$ 0.7	20.1 $\pm$ 1.2	Sy1.9	0.0760	370.6	0.107	1.3 (0.1-2.4)
	^*	[6.2 $\pm$ 0.9]	[28.0 $\pm$ 1.4]					24 (20-100)
1RXS J191928.5-295808	^*	42 $\pm$ 8	122 $\pm$ 6	Sy1.5/1.8	0.1669	863.5	0.139	12 (0.1-2.4)
	^*	[56 $\pm$ 11]	[183 $\pm$ 9]					120 (17-60)
								67 (20-40)
								<42 (40-100)
1RXS J211928.4+333259	^*	10 $\pm$ 2	15.2 $\pm$ 0.8	Sy1.5	0.051	244.4	0.217	0.44 (0.1-2.4)
	^*	[18 $\pm$ 3]	[29.6 $\pm$ 1.5]					6.8 (0.2-12)
								5.6 (14-150)
								11 (14-195)
								9.1 (17-60)
								11 (20-100)
1RXS J213944.3+595016	^*	3.0 $\pm$ 0.2	2.01 $\pm$ 0.10	Sy1.5	0.114	570.4	1.271	1.7 (0.1-2.4)
	^*	[112 $\pm$ 8]	[72 $\pm$ 4]					23 (2-10)
								14 (14-150)
								40 (20-100)
IGR J22292+6647	^*	2.25 $\pm$ 0.11	1.24 $\pm$ 0.06	Sy1.5	0.112	559.6	1.089	0.63 (0.1-2.4)
	^*	[52 $\pm$ 3]	[26.3 $\pm$ 1.3]					12 (0.2-12)
								25 (2-10)
								55 (14-150)
								100 (14-195)
								42 (17-60)
								42 (20-100)

Notes. Emission-line fluxes are reported both as observed and (between square brackets) corrected for the intervening Galactic absorption $E(B-V)_{\rm Gal}$ along the object line of sight (from Schlegel et al. 1998). Line fluxes are in units of 10^-15 erg cm^-2 s^-1, whereas X-ray luminosities are in units of 10⁴³ erg s^-1 and the reference band (between round brackets) is expressed in keV. The typical error in the redshift measurement is $\pm$ 0.001 but for the SDSS and 6dFGS spectra, for which an uncertainty of $\pm$ 0.0003 can be assumed.
^(*) Heavily blended with [N II] lines.

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