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Table 1.

Summary of selected lensing clusters.

Cluster RA Dec zcl Notes Model reference
(J2000) (J2000)
Abell 2744 00:14:20.702 −30:24:00.63 0.308 MACS, FF Jauzac et al. (2015)
Abell 370 02:39:53.122 −01:34:56.14 0.375 FF Richard et al. (2010)
MACS J0257.6−2209 02:57:41.070 −22:09:17.70 0.322 MACS Repp & Ebeling (2018)
MACS J0329.6−0211 03:29:41.568 −02:11:46.41 0.450 MACS, CLASH Zitrin et al. (2012)
MACS J0416.1−2403 04:16:09.144 −24:04:02.95 0.397 MACS, CLASH, FF Jauzac et al. (2014)
1E 0657−56 (Bullet) 06:58:38.126 −55:57:25.87 0.296 Paraficz et al. (2016)
MACS J0940.9+0744 09:40:53.698 +07:44:25.31 0.335 MACS Leethochawalit et al. (2016)
MACS J1206.2−0847 12:06:12.149 −08:48:03.37 0.438 MACS, CLASH Ebeling et al. (2009)
RX J1347.5−1145 13:47:30.617 −11:45:09.51 0.451 MACS, CLASH Halkola et al. (2008)
SMACS J2031.8−4036 20:31:53.256 −40:37:30.79 0.331 MACS Christensen et al. (2012)
SMACS J2131.1−4019 21:31:04.831 −40:19:20.92 0.442 MACS Repp & Ebeling (2018)
MACS J2214.9−1359 22:14:57.292 −14:00:12.91 0.502 MACS Ebeling et al. (2007)

Notes. The reference WCS location corresponds to the brightest cluster member of the (sub-)cluster targetted by the MUSE observations. We mention in the notes whether the target belongs to the MACS, Frontier Fields (Lotz et al. 2017) or CLASH (Postman et al. 2012) surveys, as well as other relevant publications about preliminary mass models or known lensed arcs in these clusters prior to the MUSE observations. The rightmost columns give the reference to the lens model used to design the MUSE observations.

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