The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching

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Volume 618 (October 2018)

A&A, 618 (2018) A140

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Table 1.

Overview of the cluster sample studied here.

				Y_X - M₅₀₀	Y_SZ - M₅₀₀	R_{500,Y_X}
Name	Redshift ^a			(10¹⁴ M_⊙)	(10¹⁴ M_⊙)	(kpc)	Alternative Name
`PSZ2 G044.77-51.30`	0.503(3/1)	22:14:57.27	−14:00:12.7				MACSJ2214.9-1359
`PSZ2 G045.32-38.46`	0.589(10/1)	21:29:26.13	−07:41:27.6				MACSJ2129.4-0741
`PSZ2 G045.87+57.70`	0.609(87/22)	15:18:20.56	+29:27:40.2
`PSZ2 G046.13+30.72`	0.569(67/17)	17:17:05.55	+24:04:23.7
`PSZ2 G070.89+49.26`	0.602(94/34)	15:56:25.24	+44:40:42.6
`PSZ2 G073.31+67.52`	0.609(110/35)	14:20:40.11	+39:55:06.9				WHL J215.168+39.91
`PSZ2 G094.56+51.03`	0.539(47/20)	15:08:21.98	+57:55:14.9				WHL J227.050+57.90
`PSZ2 G099.86+58.45`	0.615(104/16)	14:14:47.20	+54:47:03.5				WHL J213.697+54.78
`PSZ2 G111.61-45.71`	0.546(388/187)	00:18:33.58	+16:26:15.9				RXC J0018.5+1626
`PSZ2 G144.83+25.11`	0.591(4/1)	06:47:50.65	+70:14:54.0				MACSJ0647.7+7015
`PLCK G147.30-16.60`^b	0.645(8/8)	02:56:23.45	+40:17:28.9				RXC J0254.4+4134
`PSZ2 G155.27-68.42`	0.567(68/24)	01:37:24.98	−08:27:22.9				WHL J24.3324-8.477
`PSZ2 G180.25+21.03`	0.546(1151/529)	07:17:35.63	+37:45:17.4				MACSJ0717.5+3745
`PSZ2 G183.90+42.99`	0.559(94/25)	09:10:51.05	+38:50:22.3				WHL J137.713+38.83
`PSZ2 G193.31-46.13`	0.634(45/2)	03:35:52.00	−06:59:23.4
`PSZ2 G201.50-27.31`	0.538(1181/278)	04:54:10.83	−03:00:51.5				MACSJ0454.1-0300
`PSZ2 G208.61-74.39`	0.718(10/5)	02:00:16.38	−24:54:51.5
`PSZ2 G211.21+38.66`	0.505(46/18)	09:11:11.52	+17:46:29.1				RXC J0911.1+1746
`PSZ2 G212.44+63.19`	0.529(56/14)	10:52:48.75	+24:16:11.3				RMJ105252.4+241530.0
`PSZ2 G219.89-34.39`	0.734(15/5)	04:54:45.32	−20:16:58.8
`PSZ2 G228.16+75.20`	0.544(585/285)	11:49:35.68	+22:23:54.7				RXC J1149.5+2224

^(a)

Notes. In parentheses, the number of spectroscopic redshifts overlapping with the region for which we have photometry, and the number of spectroscopic cluster members (within 3000 km s⁻¹ from the cluster mean redshift), respectively.

^(b)

Cluster detected at a significance slightly below the cut-off value used for the PSZ2 catalogue. The Y_SZ is measured on the final Planck maps.

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