Compton-thick AGN in the 70-month Swift-BAT All-Sky Hard X-ray Survey: A Bayesian approach

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Volume 594 (October 2016)

A&A, 594 (2016) A73

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Table A.1

Detection and optical counterpart information of Compton-thick candidates from Baumgartner et al. (2013).

Name¹	BAT No²	S/N³	z ⁴	RA⁵	Dec⁵	Clas⁶	Ref.⁷

2MASXJ00253292+6821442	13	7.45	0.0120	6.3870	68.3623	5	–
MCG-07-03-007	49	6.22	0.0302	16.3617	–42.2162	5	a
3C033	57	13.13	0.0597	17.2203	13.3372	5	–
NGC 424	58	11.43	0.0118	17.8650	–38.0830	4	a, b
MCG+08-03-018	70	7.60	0.0204	20.6435	50.0550	5	a
ESO244-IG030	81	6.06	0.0256	22.4636	–42.3265	5	a
ARP318	112	5.60	0.0132	32.3805	–10.1585	5	–
NGC 1068	144	15.64	0.0038	40.6696	–0.0133	5	a, c
2MFGC02280	151	8.98	0.0152	42.6775	54.7049	5	a
NGC 1106	152	6.59	0.0145	42.6688	41.6715	5	a
NGC 1125	153	7.98	0.0110	42.9180	–16.6510	5	a
NGC 1194	163	13.85	0.0136	45.9546	–1.1037	4	a, d
NGC 1229	165	4.96	0.0360	47.0449	–22.9608	5	a
2MASXJ03561995-6251391	199	7.33	0.1076	59.0830	–62.8610	5	a
ESO005-G004	319	13.06	0.0064	91.4235	–86.6319	5	a, e
Mrk 3	325	55.96	0.0135	93.9015	71.0375	5	a
ESO426-G002	330	10.53	0.0224	95.9434	–32.2166	5	–
2MASXJ06561197-4919499	350	5.65	0.0410	104.0498	–49.3306	5	a
MCG+06-16-028	362	6.08	0.0157	108.5161	35.2793	5	a
Mrk 78	383	4.95	0.0371	115.6739	65.1771	5	a
2MASXJ08434495+3549421	430	5.65	0.0540	130.9375	35.8283	5	–
NGC 2788A	440	8.05	0.0133	135.6640	–68.2270	2	a
SBS0915+556	450	4.91	0.1234	139.8050	55.4653	5	a
2MASXJ09235371-3141305	456	11.29	0.0424	140.9739	–31.6919	5	a
MCG+10-14-025	467	4.83	0.0394	143.9652	61.3531	4	a
NGC 3081	480	30.41	0.0080	149.8731	–22.8263	5	q
NGC 3079	484	17.23	0.0037	150.4908	55.6798	5	a
ESO317-G041	499	8.45	0.0193	157.8463	–42.0606	2	a
SDSSJ103315.71+525217.8	505	5.96	0.0653	158.3159	52.8716	2	a
NGC 3393	518	8.95	0.0125	162.0977	–25.1621	5	a, f
NGC 3588NED01	533	5.00	0.0262	168.5103	20.3873	2	–
IC0751	580	6.23	0.0312	179.7191	42.5703	5	t
NGC 4102	590	14.77	0.0028	181.5963	52.7109	6	a, s
NGC 4180	599	6.90	0.0070	183.2620	7.0380	6	a
CGCG187-022	600	7.02	0.0249	183.2888	32.5964	5	–
NGC 4941	653	8.53	0.0037	196.0547	–5.5516	5	r
NGC 4945	655	79.31	0.0019	196.3645	–49.4682	5	a, g
Circinus Galaxy	711	110.71	0.0014	213.2913	–65.3390	6	a, h
IGRJ14175-4641	714	8.34	0.0760	214.2652	–46.6948	5	a, i
NGC 5643	731	5.40	0.0040	218.1699	–44.1746	5	a, j
NGC 5728	739	24.34	0.0093	220.5997	–17.2532	5	a, k
CGCG164-019	740	5.08	0.0299	221.4035	27.0348	5	a
ESO137-G034	823	8.44	0.0090	248.8070	–58.0800	5	a, l
NGC 6232	828	5.05	0.0290	250.8343	70.6325	2	a
NGC 6240	841	18.82	0.0245	253.2454	2.4009	5	a, m
NGC 6552	942	19.19	0.0265	270.0304	2.4009	5	a
2MASXJ20145928+2523010	1070	5.38	0.0453	303.7470	25.3836	6	a
MCG+04-48-002	1077	26.74	0.0139	307.1461	66.6154	5	a
ESO234-IG063	1087	5.94	0.0537	310.0656	–51.4297	5	–
NGC 7130	1127	5.31	0.0162	327.0813	–34.9512	5	a, n
NGC 7212NED02	1139	4.87	0.0267	331.7582	10.2334	4	a, o
NGC 7479	1184	7.02	0.0079	346.2361	12.3229	5	a, p
2MASXJ23222444-0645375	1192	5.56	0.0330	350.6019	–6.7605	5	–

Notes.

⁽¹⁾

Name of the optical counterpart;

⁽²⁾

reference number in the Swift-BAT catalogue;

⁽³⁾

signal-to-noise ratio in the 14−195 keV band;

⁽⁴⁾

redshift;

⁽⁵⁾

coordinates of the optical counterpart of the BAT source;

⁽⁶⁾

optical classification index of the sources: class 2 = Galaxies, class 4 = Seyfert I, class 5 = Seyfert II, class 6 = “other AGN”;

⁽⁷⁾

recent papers presenting evidence for Compton thickness: a = Ricci et al. (2015), b = Baloković et al. (2014), c = Marinucci et al. (2016), d = Greenhill et al. (2008), e = Ueda et al. (2007), f = Koss et al. (2015), g = Puccetti et al. (2014), h = Arévalo et al. (2014), i = Malizia et al. (2009), j = Annuar et al. (2015), k = Comastri et al. (2010), l = Burtscher et al. (2015), m = Puccetti et al. (2016), n = González-Martín et al. (2009), o = Hernández-García et al. (2015), p = Georgantopoulos et al. (2011), q = Eguchi et al. (2011), r = Salvati et al. (1997), s = González-Martín et al. (2011), t = Ricci et al. (2016).

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