Occurrence of radio halos in galaxy clusters - Insight from a mass-selected sample

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Volume 580 (August 2015)

A&A, 580 (2015) A97

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Table 1

Total sample clusters properties.

Cluster name	RA	Dec	z	M₅₀₀	Radio info	X-ray info
				(10¹⁴ M_⊙)


A1437	12 00 22.3	+03 20 33.9	0.134	5.69	no RH^*	M √
A2345	21 27 06.8	−12 07 56.0	0.176	5.71	Relics⁴	M √
A2104	15 40 08.2	−03 18 23.0	0.153	5.91	no RH^*	M √
Zwcl 2120.1+2256	21 22 27.1	+23 11 50.3	0.143	5.91	no RH^*	M √
RXC J0616.3-2156	06 16 22.8	−21 56 43.4	0.171	5.93	no RH^*	M √
A1413	11 55 18.9	+23 24 31.0	0.143	5.98	MH⁵	R √
A1576	12 37 59.0	+63 11 26.0	0.302	5.98	UL⁶	R²⁶
A2697	00 03 11.8	−06 05 10.0	0.232	6.01	UL²	R^x
Z5247	12 33 56.1	+09 50 28.0	0.229	6.04	RH⁷	M √
Zwcl 0104.9+5350	01 07 54.0	+54 06 00.0	0.107	6.06	RH⁸	–
RXC J0142.0+2131	01 42 02.6	+21 31 19.0	0.280	6.07	UL⁶	R²⁶
A1423	11 57 22.5	+33 39 18.0	0.214	6.09	UL²	R²⁵
RXC J1314.4-2515	13 14 28.0	−25 15 41.0	0.244	6.15	RH¹	M^x
A2537	23 08 23.2	−02 11 31.0	0.297	6.17	UL²	R²⁵
A68	00 37 05.3	+09 09 11.0	0.255	6.19	UL⁷	M √
A1682	13 06 49.7	+46 32 59.0	0.226	6.20	RH²	M²⁵
A1132	10 58 19.6	+56 46 56.0	0.134	6.23	no RH³	M √
RXJ1720.1+2638	17 20 10.1	+26 37 29.5	0.164	6.34	MH⁹	R √
A781	09 20 23.2	+30 26 15.0	0.295	6.36	UL²	M²⁵
A2218	16 35 51.6	+66 12 39.0	0.171	6.41	RH³	M²⁸√
A3411	08 41 55.6	−17 29 35.7	0.169	6.48	RH¹⁰	M √
Zwcl 0634.1+4750	06 38 02.5	+47 47 23.8	0.174	6.52	suspect^*	M √
A3888	22 34 26.8	−37 44 19.1	0.151	6.67	suspect^*	M?^x²⁹
A3088	03 07 04.1	−28 40 14.0	0.254	6.71	UL²	R²⁶
A2667	23 51 40.7	−26 05 01.0	0.226	6.81	UL²	R²⁵
A521	04 54 09.1	−10 14 19.0	0.248	6.91	RH¹¹^US	M²⁵
A2631	23 37 40.6	+00 16 36.0	0.278	6.97	UL²	M²⁵
A1914	14 26 03.0	+37 49 32.0	0.171	6.97	RH¹²	M √
RXC J1504.1-0248	15 04 07.7	−02 48 18.0	0.215	6.98	MH¹³	R²⁵
A520	04 54 19.0	+02 56 49.0	0.203	7.06	RH¹⁴	M²⁵
A478	04 13 20.7	+10 28 35.0	0.088	7.06	MH¹⁵	R √
A773	09 17 59.4	+51 42 23.0	0.217	7.08	RH¹⁴	M²⁵
A1351	11 42 30.8	+58 32 20.0	0.322	7.14	RH¹⁶	M √
A115	00 55 59.5	+26 19 14.0	0.197	7.21	Relic¹⁴	M √
A1451	12 03 16.2	−21 32 12.7	0.199	7.32	suspect^*	M^x
PSZ1 G205.07-62.94	02 46 27.5	−20 32 5.29	0.310	7.37	no RH^p	M^x
A2261	17 22 17.1	+32 08 02.0	0.224	7.39	UL⁶	R²⁵
RXCJ2003.5-2323	20 03 30.4	−23 23 05.0	0.317	7.48	RH¹	M²⁵
A2552	23 11 26.9	+03 35 19.0	0.300	7.53	RH?⁷	R? √
A3444	10 23 50.8	−27 15 31.0	0.254	7.62	MH⁷	R √
S780	14 59 29.3	−18 11 13.0	0.236	7.71	MH⁷	R²⁵
A2204	16 32 45.7	+05 34 43.0	0.151	7.96	MH¹⁵	R √
A1758a	13 32 32.1	+50 30 37.0	0.280	7.99	RH¹⁷	M²⁵
A209	01 31 53.0	−13 36 34.0	0.206	8.17	RH¹	M²⁵
A665	08 30 45.2	+65 52 55.0	0.182	8.23	RH³	M √
A1763	13 35 17.2	+40 59 58.0	0.228	8.29	no RH²	M √
RXC J1514.9-1523	15 14 58.0	−15 23 10.0	0.223	8.34	RH¹⁸^c	M √
A1835	14 01 02.3	+02 52 48.0	0.253	8.46	MH¹⁹	R √
A2142	15 58 16.1	+27 13 29.0	0.089	8.81	RH²⁴	M³⁰√
A1689	13 11 29.5	−01 20 17.0	0.183	8.86	RH²⁰	M²⁷√
A1300	11 31 56.3	−19 55 37.0	0.308	8.83	RH²¹^c	M²⁵
A2390	21 53 34.6	+17 40 11.0	0.234	9.48	MH¹²	R²⁵
A2744	00 14 18.8	−30 23 00.0	0.307	9.56	RH¹⁴	M²⁵
A2219	16 40 21.1	+46 41 16.0	0.228	11.01	RH¹²	M²⁵
PSZ1 G171.96-40.64	03 12 57.4	+08 22 10	0.270	11.13	RH²²^c	M^x
A697	08 42 53.3	+36 20 12.0	0.282	11.48	RH³²^US	M²⁵³¹
A2163	16 15 46.9	−06 08 45.0	0.203	16.44	RH²³	M²⁵

Notes. RH = Radio Halo, MH = Mini-Halo, UL = Upper Limit, M = merger, R = relaxed.

Reference.

⁽¹⁾

Venturi et al. (2007);

⁽²⁾

Venturi et al. (2008);

⁽³⁾

Giovannini & Feretti (2000);

⁽⁴⁾

Bonafede et al. (2009);

⁽⁵⁾

Govoni et al. (2009);

⁽⁶⁾

Kale et al. (2013);

⁽⁷⁾

Kale et al. (2015);

⁽⁸⁾

van Weeren et al. (2011);

⁽⁹⁾

Giacintucci et al. (2014b);

⁽¹⁰⁾

van Weeren et al. (2013);

⁽¹¹⁾

Brunetti et al. (2008);

⁽¹²⁾

Bacchi et al. (2003);

⁽¹³⁾

Giacintucci et al. (2011a);

⁽¹⁴⁾

Govoni et al. (2001);

⁽¹⁵⁾

Giacintucci et al. (2014a);

⁽¹⁶⁾

Giacintucci et al. (2009);

⁽¹⁷⁾

Giovannini et al. (2006);

⁽¹⁸⁾

Giacintucci et al. (2011b);

⁽¹⁹⁾

Murgia et al. (2009);

⁽²⁰⁾

Vacca et al. (2011);

⁽²¹⁾

Venturi et al. 2013;

⁽²²⁾

Giacintucci et al. (2013);

⁽²³⁾

Feretti et al. (2001);

⁽²⁴⁾

Farnsworth et al. (2013);

⁽²⁵⁾

Cassano et al. (2010);

⁽²⁶⁾

Cassano et al. (2013);

⁽²⁷⁾

Andersson & Madejski (2004);

⁽²⁸⁾

Pratt et al. (2005);

⁽²⁹⁾

Weißmann et al. (2013a);

⁽³⁰⁾

Owers et al. (2011);

⁽³¹⁾

Girardi et al. (2006);

⁽³²⁾

Macario et al. 2010;

^(US)

Ultra Steep Spectrum RH;

^(c)

candidate USSRH;

^(p)

Ferrari et al. (priv. comm.);

^(x)

visual inspection of XMM-Newton image;

^(*)

NVSS data analysed in this paper; (√) X-ray Chandra data analysed in this paper.

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