Constraints on the alignment of galaxies in galaxy clusters from ~14 000 spectroscopic members

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Table 2

Cluster sample, redshifts, and velocity dispersions.

Cluster	z	N _m	N ₂₀₀	σ ₂₀₀	M ₂₀₀	r ₂₀₀		Main	Main NED
				(km s^-1)	(10¹⁴ M_⊙)	(Mpc)		sources^a	sources^b

Abell 85	0.0555	284	248	967 ± 55	10.0 ± 1.7	2.03 ± 0.12	(D)	3	14
Abell 115	0.1930	73	73	1028 ± 108	11.2 ± 3.5	2.03 ± 0.21	(R)	–	1
Abell 119	0.0443	268	255	875 ± 48	7.5 ± 1.2	1.85 ± 0.10	<0.01(D)	3	7
Abell 133	0.0558	62	59	791 ± 79	5.5 ± 1.7	1.66 ± 0.17	(R)	–	21
Abell 209^c	0.2090	110	110	1170 ± 99	16.4 ± 4.1	2.28 ± 0.19	(D)	–	27
Abell 222^c	0.2132	76	76	881 ± 79	7.0 ± 1.9	1.72 ± 0.15	(R)	–	11, 33
Abell 223^c	0.2076	64	64	910 ± 80	7.8 ± 2.1	1.78 ± 0.16	(D)	–	11, 33
Abell 267	0.2291	219	156	1006 ± 74	10.3 ± 2.3	1.95 ± 0.14	<0.01(D)	3, 4	–
Abell 2670	0.0763	241	196	919 ± 46	8.5 ± 1.3	1.91 ± 0.10	<0.01(D)	3	21
Abell 2703	0.1140	75	13	657 ± 53	3.1 ± 0.8	1.35 ± 0.11	(R)	3	–
Abell 383	0.1885	182	134	918 ± 53	8.1 ± 1.4	1.81 ± 0.11	<0.01(D)	–	18
Abell 399	0.0718	250	229	1046 ± 47	12.5 ± 1.7	2.18 ± 0.10	<0.01(D)	5	20
Abell 401	0.0735	104	83	933 ± 81	8.9 ± 2.3	1.94 ± 0.17	(R)	–	20
Abell 520	0.2007	153	127	1045 ± 73	11.8 ± 2.5	2.05 ± 0.14	(R)	–	19
Abell 521^c	0.2469	95	95	1002 ± 95	10.1 ± 2.9	1.92 ± 0.18	(D)	–	16
Abell 545^c	0.1577	80	80	1038 ± 89	11.8 ± 3.0	2.08 ± 0.18	(R)	–	2
Abell 553	0.0670	54	44	665 ± 75	3.3 ± 1.1	1.39 ± 0.16	(D)	5	–
Abell 586	0.1704	33	21	803 ± 104	5.4 ± 2.1	1.60 ± 0.21	(R)	3	–
Abell 644^c	0.0696	31	31	625 ± 96	2.7 ± 1.2	1.31 ± 0.20	(R)	–	24
Abell 646	0.1266	259	69	707 ± 66	3.8 ± 1.1	1.44 ± 0.13	(D)	3, 4	–
Abell 655	0.1271	306	109	938 ± 57	8.8 ± 1.6	1.91 ± 0.12	(D)	3, 4	–
Abell 697	0.2821	215	106	1161 ± 89	15.4 ± 3.6	2.19 ± 0.17	(R)	3, 4	–
Abell 754	0.0546	305	300	959 ± 43	9.8 ± 1.3	2.01 ± 0.09	(D)	–	8
Abell 780^c	0.0547	33	33	822 ± 113	6.2 ± 2.5	1.73 ± 0.24	(D)	–	21
Abell 795	0.1385	166	117	768 ± 59	4.9 ± 1.1	1.56 ± 0.12	(D)	3, 4, 5	–
Abell 851	0.4038	53	47	999 ± 138	9.3 ± 3.8	1.77 ± 0.24	(D)	–	3, 12
Abell 959	0.2882	67	67	982 ± 101	9.4 ± 2.9	1.85 ± 0.19	(D)	–	5
Abell 961	0.1275	58	16	740 ± 142	4.4 ± 2.5	1.51 ± 0.29	(R)	3	–
Abell 963	0.2036	165	85	922 ± 64	8.1 ± 1.7	1.81 ± 0.13	(R)	3, 4	–
Abell 990	0.1421	209	86	829 ± 96	6.1 ± 2.1	1.68 ± 0.19	(R)	3, 4, 5	–
Abell 1033	0.1224	170	98	762 ± 52	4.8 ± 1.0	1.56 ± 0.11	(R)	3, 4	–
Abell 1068	0.1393	104	32	740 ± 160	4.3 ± 2.8	1.50 ± 0.32	(R)	3, 4	–
Abell 1132	0.1349	160	55	727 ± 89	4.1 ± 1.5	1.48 ± 0.18	(R)	3, 4	–
Abell 1234	0.1638	54	30	513 ± 86	1.4 ± 0.7	1.03 ± 0.17	(R)	3, 4	–
Abell 1246	0.1920	207	87	956 ± 84	9.1 ± 2.4	1.89 ± 0.17	(D)	3, 4	–
Abell 1285	0.1078	77	51	826 ± 90	6.1 ± 2.0	1.70 ± 0.19	(R)	5	–
Abell 1361	0.1157	143	46	587 ± 62	2.2 ± 0.7	1.21 ± 0.13	(R)	3, 4	–
Abell 1413	0.1418	124	65	881 ± 81	7.3 ± 2.0	1.78 ± 0.16	(R)	3, 4	–
Abell 1650	0.0841	266	140	720 ± 48	4.1 ± 0.8	1.50 ± 0.10	(R)	3, 5	–
Abell 1651	0.0847	214	138	903 ± 51	8.0 ± 1.4	1.87 ± 0.11	(R)	–	9, 21
Abell 1689	0.1847	252	235	1429 ± 81	30.0 ± 5.1	2.82 ± 0.16	<0.01(D)	3, 4	–
Abell 1758	0.2772	133	34	744 ± 107	4.1 ± 1.8	1.41 ± 0.20	(R)	3, 4	–
Abell 1763	0.2323	186	103	1130 ± 81	14.6 ± 3.1	2.18 ± 0.16	<0.01(D)	3, 4	–
Abell 1781	0.0622	54	16	419 ± 93	0.8 ± 0.5	0.88 ± 0.19	(R)	3	–
Abell 1795	0.0629	191	133	778 ± 51	5.2 ± 1.0	1.63 ± 0.11	(R)	3	21
Abell 1835	0.2506	195	41	762 ± 106	4.5 ± 1.9	1.46 ± 0.20	(R)	3, 4	–
Abell 1914	0.1671	257	146	911 ± 54	7.9 ± 1.4	1.82 ± 0.11	(R)	3, 4	–
Abell 1927	0.0953	138	58	725 ± 58	4.2 ± 1.0	1.50 ± 0.12	(R)	3, 5	–
Abell 1942	0.2257	51	27	820 ± 140	5.6 ± 2.9	1.59 ± 0.27	(D)	3	–
Abell 1991	0.0587	175	99	553 ± 45	1.9 ± 0.5	1.17 ± 0.10	(R)	3, 5	–
Abell 2029	0.0777	317	181	1152 ± 58	16.6 ± 2.5	2.39 ± 0.12	<0.01(D)	3	21
Abell 2033	0.0796	190	88	911 ± 69	8.3 ± 1.9	1.89 ± 0.14	(D)	3	21
Abell 2050	0.1202	164	82	854 ± 80	6.7 ± 1.9	1.74 ± 0.16	(R)	3, 4	–
Abell 2055	0.1028	154	69	697 ± 64	3.7 ± 1.0	1.44 ± 0.13	(D)	3, 4	21
Abell 2064	0.0734	62	32	675 ± 108	3.4 ± 1.6	1.41 ± 0.22	(R)	3	–
Abell 2065	0.0725	219	164	1095 ± 67	14.3 ± 2.6	2.28 ± 0.14	(D)	3	–
Abell 2069	0.1139	331	146	966 ± 63	9.7 ± 1.9	1.98 ± 0.13	(D)	3, 4	–
Abell 2104	0.1547	90	56	1081 ± 126	13.3 ± 4.6	2.17 ± 0.25	(R)	–	23
Abell 2111	0.2281	256	83	738 ± 66	4.1 ± 1.1	1.43 ± 0.13	(R)	3, 4	29
Abell 2125	0.2466	141	55	857 ± 122	6.4 ± 2.7	1.65 ± 0.23	(R)	–	28
Abell 2142	0.0903	1052	731	1086 ± 31	13.9 ± 1.2	2.24 ± 0.06	(D)	3	31
Abell 2163	0.2004	309	290	1279 ± 53	21.5 ± 2.7	2.51 ± 0.10	(D)	–	25
Abell 2204	0.1507	100	15	782 ± 278	5.1 ± 5.4	1.58 ± 0.56	(R)	–	32
Abell 2219	0.2255	364	241	1189 ± 65	17.0 ± 2.8	2.30 ± 0.13	<0.01(D)	3, 4	4
Abell 2259	0.1602	158	77	901 ± 70	7.7 ± 1.8	1.80 ± 0.14	(D)	3, 4	–
Abell 2261	0.2257	206	76	882 ± 86	7.0 ± 2.0	1.71 ± 0.17	(D)	3, 4	–
Abell 2319^c	0.0538	83	83	1101 ± 99	14.7 ± 4.0	2.31 ± 0.21	(R)	–	30
Abell 2390	0.2287	136	92	1120 ± 113	14.3 ± 4.3	2.17 ± 0.22	(R)	2	–
Abell 2409	0.1454	101	46	826 ± 94	6.0 ± 2.0	1.67 ± 0.19	(R)	3, 5	–
Abell 2440^c	0.0906	88	88	766 ± 61	4.9 ± 1.2	1.59 ± 0.13	(R)	3	26
Abell 2495	0.0790	98	46	631 ± 55	2.8 ± 0.7	1.32 ± 0.12	(R)	3, 5	–
Abell 2537	0.2964	175	65	909 ± 85	7.4 ± 2.1	1.70 ± 0.16	(D)	3	6
Abell 2597	0.0829	39	17	682 ± 131	3.5 ± 2.0	1.42 ± 0.27	(R)	–	9, 13
CL 0024.0+1652	0.3948	229	131	757 ± 48	4.1 ± 0.8	1.35 ± 0.09	<0.01(D)	–	10
MACS J0717.5+3745	0.5436	468	215	1370 ± 79	22.0 ± 3.8	2.24 ± 0.13	<0.01(D)	–	15
MKW3S	0.0444	125	82	592 ± 49	2.3 ± 0.6	1.25 ± 0.11	(R)	3	–
MS 0015.9+1609	0.5475	232	122	1330 ± 115	20.0 ± 5.2	2.17 ± 0.19	(R)	1, 2	–
MS 0440.5+0204	0.1962	51	35	742 ± 103	4.3 ± 1.8	1.46 ± 0.20	(R)	2	–
MS 0451.6−0305	0.5382	247	200	1252 ± 55	16.8 ± 2.2	2.05 ± 0.09	<0.01(D)	1, 2	–
MS 1008.1−1224	0.3077	86	85	1028 ± 92	10.6 ± 2.8	1.91 ± 0.17	(R)	2	22
MS 1224.7+2007	0.3258	33	29	790 ± 95	4.8 ± 1.7	1.46 ± 0.17	(R)	2, 3	–
MS 1231.3+1542	0.2347	84	65	710 ± 57	3.7 ± 0.9	1.38 ± 0.11	(R)	2, 3	–
MS 1358.4+6245	0.3289	189	152	1021 ± 56	10.3 ± 1.7	1.88 ± 0.10	(D)	2	17
MS 1455.0+2232	0.2565	57	57	928 ± 111	8.0 ± 2.9	1.77 ± 0.21	(R)	2, 3	–
MS 1512.4+3647	0.3719	30	29	960 ± 170	8.4 ± 4.4	1.73 ± 0.30	(D)	2	–
MS 1621.5+2640	0.4254	70	41	724 ± 82	3.5 ± 1.2	1.27 ± 0.14	(R)	2	–
RX J0736.6+3924	0.1179	62	28	432 ± 64	0.9 ± 0.4	0.89 ± 0.13	(R)	3, 5	–
ZwCl 0628.1+2502	0.0814	72	66	843 ± 96	6.6 ± 2.2	1.75 ± 0.20	(D)	5	–
ZwCl 1023.3+1257	0.1425	84	24	622 ± 108	2.6 ± 1.3	1.26 ± 0.22	(R)	3, 4	–
ZwCl 1215.1+0400	0.0773	183	107	902 ± 65	8.0 ± 1.7	1.88 ± 0.14	(R)	3	–

Notes. Columns are: (1) cluster name; (2) cluster redshift; (3) number of members out to arbitrary radius; (4) number of members within r₂₀₀; (5) velocity dispersion of members within r₂₀₀; (6) total mass within r₂₀₀; (7) cluster radius r₂₀₀; (8) significance level of the DS test, the letter in parenthesis shows whether a cluster is classified as disturbed (D), relaxed (R), or intermediate (I).

^(a)

Numbers are: (1) WLTV; (2) CNOC; (3) SDSS; (4) HeCS; (5) MENeaCS-spec. See text for references.

^(b)

Catalogs extracted from NED that contribute significantly to each cluster. These are: (1) Barrena et al. (2007); (2) Barrena et al. (2011); (3) Belloni & Roser (1996); (4) Boschin et al. (2004); (5) Boschin et al. (2009); (6) Braglia et al. (2009); (7) WINGS (Cava et al. 2009); (8) Christlein & Zabludoff (2003); (9) 2dF (Colless et al. 2003); (10) Czoke et al. (2001); (11) Dietrich et al. (2002); (12) Dressler & Gunn (1992); (13) WiggleZ (Drinkwater et al. 2010); (14) Durret et al. (1998); (15) Ebeling et al. (2014); (16) Ferrari et al. (2003); (17) Fisher et al. (1998); (18) Geller et al. (2014); (19) Girardi et al. (2008); (20) Hill & Oegerle (1993); (21) 2MRS (Huchra et al. 2012); (22) Jäger et al. (2004); (23) Liang et al. (2000); (24) Martini et al. (2007); (25) Maurogordato et al. (2008); (26) Maurogordato et al. (2011); (27) Mercurio et al. (2003); (28) Miller et al. (2004); (29) Miller et al. (2006); (30) Oegerle et al. (1995); (31) Owers et al. (2011); (32) Pimbblet et al. (2006); (33) Proust et al. (2000).

^(c)

Spectroscopic members extend out to less than 0.8r₂₀₀.

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