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

Home

All issues

Volume 519 (September 2010)

A&A, 519 (2010) A96

Full HTML

Free Access

Table 5:

Synoptic table containing the main results concerning the 13 narrow emission-line AGNs and of the single XBONG (see Figs. 11-13) 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	E(B-V)		$L_{\rm X}$
						(Mpc)	Gal.	AGN
IGR J00465-4005	1.8 $\pm$ 0.4	0.17 $\pm$ 0.05	3.63 $\pm$ 0.18	Sy2	0.201	1061.3	0.011	1.26	16 (2-10)
	[2.1 $\pm$ 0.6]	[0.21 $\pm$ 0.07]	[3.71 $\pm$ 0.19]						480 (20-100)
IGR J01545+6437	27 $\pm$ 3	2.6 $\pm$ 0.3	17.0 $\pm$ 0.9	Sy2	0.034	160.9	0.866	0.38	1.4 (20-40)
	[170 $\pm$ 20]	[41 $\pm$ 5]	[240 $\pm$ 12]						<1.2 (40-100)
IGR J03344+1506	42 $\pm$ 2	5.1 $\pm$ 0.5	20.7 $\pm$ 1.0	Sy2	0.021	98.4	0.316	0.81	0.0095 (0.1-2.4)
	[87 $\pm$ 4]	[14.0 $\pm$ 1.4]	[54 $\pm$ 3]						<0.79 (20-40)
									2.3 (40-100)
IGR J04451-0445	5.2 $\pm$ 0.5	<0.5	<0.7	likely Sy2	0.076	370.6	0.048	>1.05	47 (20-100)
	[5.6 $\pm$ 0.3]	[<0.7]	[<0.9]
IGR J05253+6447	4.5 $\pm$ 0.5	in abs.	6.0 $\pm$ 0.3	likely Sy2	0.071	345.0	0.190	--	7.7 (0.2-2)
	[6.7 $\pm$ 0.7]	''	[11.1 $\pm$ 0.6]						<8.6 (20-40)
									19 (40-100)
IGR J06293-1359	34.8 $\pm$ 1.7	3.3 $\pm$ 0.2	19.0 $\pm$ 0.6	Sy2	0.033	156.0	0.323	1.28	4.8 (20-40)
	[73 $\pm$ 4]	[7.4 $\pm$ 0.5]	[51.7 $\pm$ 1.6]						<4.1 (40-100)
IGR J08557+6420	6.2 $\pm$ 0.4	in abs.	8.8 $\pm$ 0.4	likely Sy2	0.037	175.5	0.103	--	7.4 (17-60)
	[7.9 $\pm$ 0.6]	''	[12.3 $\pm$ 0.6]
MCG +04-26-006	21 $\pm$ 2	8.2 $\pm$ 0.6	15.4 $\pm$ 0.8	LINER	0.020	93.7	0.030	0	0.23 (2-10)
	[22 $\pm$ 2]	[8.6 $\pm$ 0.6]	[17.0 $\pm$ 0.9]						1.4 (14-150)
									3.3 (20-100)
IGR J14301-4158	22.5 $\pm$ 1.8	5.7 $\pm$ 0.9	39.6 $\pm$ 1.2	Sy2	0.0387	183.8	0.117	0.29	3.7 (20-100)
	[29 $\pm$ 2]	[7.6 $\pm$ 1.2]	[56.1 $\pm$ 1.7]
IGR J15549-3740	67.7 $\pm$ 1.8	7.93 $\pm$ 0.12	46 $\pm$ 2	Sy2	0.0194	90.8	0.475	0.67	1.7 (20-100)
	[200 $\pm$ 6]	[36 $\pm$ 5]	[195 $\pm$ 10]
IGR J17009+3559	--	in abs.	<0.33	XBONG	0.113	565.0	0.018	--	8.0 (1-10)
	--	''	[<0.34]						52 (17-60)
IGR J18308+0928	13.1 $\pm$ 1.3	<2	16.0 $\pm$ 1.6	Sy2	0.019	88.9	0.243	>0.83	1.5 (14-150)
	[26 $\pm$ 3]	<4	[33 $\pm$ 3]						3.7 (14-195)
									0.081 (17-60)
IGR J18311-3337	40.2 $\pm$ 1.8	6.0 $\pm$ 0.6	82 $\pm$ 2	Sy2	0.0687	333.3	0.185	0.94	22 (20-100)
	[60 $\pm$ 3]	[8.4 $\pm$ 0.8]	[141 $\pm$ 4]
IGR J19118-1707	132 $\pm$ 4	32 $\pm$ 2	83 $\pm$ 4	LINER	0.0234	109.9	0.137	0.25	0.87 (20-40)
	[179 $\pm$ 5]	49 $\pm$ 3	[126 $\pm$ 6]						<0.82 (40-100)

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.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.