Table 1.
Summary of the 17 galaxy clusters.
| Cluster | RA | Dec. | zcl | MUSE depth | N pointings | N LAEs | Veff, μ > 1.5 | Veff, μ > 5.4 |
|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | [h] | [Mpc3] | [Mpc3] | ||||
| Abell 2744 | 00:14:20.702 | −30:24:00.63 | 0.308 | 3.5–7 | 4 | 142 (121) | 5080.4 | 84.4 |
| Abell 370 | 02:39:53.122 | −01:34:56.14 | 0.375 | 1.5–8.5 | 4 | 98 (42) | 3566.5 | 216.8 |
| MACS J0257.6−2209 | 02:57:41.070 | −22:09:17.70 | 0.322 | 8 | 1 | 48 (25) | 711.7 | 76.9 |
| MACS J0329.6−0211 | 03:29:41.568 | −02:11:46.41 | 0.450 | 2.5 | 1 | 8 (17) | 1155.8 | 63.9 |
| MACS J0416.1−2403 N | 04:16:09.144 | −24:04:02.95 | 0.397 | 17 | 1 | 71 (46) | 1330.0 | 45.3 |
| MACS J0416.1−2403 S | 04:16:09.144 | −24:04:02.95 | 0.397 | 11–15 | 1 | 56 (34) | 1330.0 | 45.3 |
| MACS J0451.9+0006 | 04:51:54.647 | +00:06:18.21 | 0.430 | 8 | 1 | 45 (21) | 863.5 | 51.3 |
| MACS J0520.7−1328 | 05:20:42.046 | −13:28:47.58 | 0.336 | 8 | 1 | 33 (19) | 696.6 | 101.4 |
| 1E 0657−56 (Bullet) | 06:58:38.126 | −55:57:25.87 | 0.296 | 2 | 1 | 14 (11) | 898.3 | 69.0 |
| MACS J0940.9+0744 | 09:40:53.698 | +07:44:25.31 | 0.335 | 8 | 1 | 58 (49) | 2310.1 | 20.2 |
| MACS J1206.2−0847 | 12:06:12.149 | −08:48:03.37 | 0.438 | 4–9 | 3 | 82 (50) | 2791.2 | 133.8 |
| RX J1347.5−1145 | 13:47:30.617 | −11:45:09.51 | 0.451 | 2–3 | 4 | 124 (72) | 2929.4 | 96.8 |
| SMACS J2031.8−4036 | 20:31:53.256 | −40:37:30.79 | 0.331 | 10 | 1 | 44 (21) | 1329.9 | 55.4 |
| SMACS J2131.1−4019 | 21:31:04.831 | −40:19:20.92 | 0.442 | 7 | 1 | 30 (16) | 586.0 | 100.3 |
| Abell 2390 | 21:53:36.823 | +17:41:43.59 | 0.228 | 2 | 1 | 14 (8) | 759.3 | 98.1 |
| MACS J2214.9−1359 | 22:14:57.292 | −14:00:12.91 | 0.502 | 7 | 1 | 33 (17) | 699.6 | 51.6 |
| Abell S1063 | 22:48:43.975 | −44:31:51.16 | 0.348 | 3.9 | 2 | 35 (20) | 1839.9 | 146.3 |
| Abell 2667 | 23:52:28.400 | −26:05:08.00 | 0.233 | 2 | 1 | 24 (14) | 820.0 | 99.0 |
| Total | 30 | 959 (603) | 29534.8 | 1556.7 | ||||
Notes. The seventh column shows the number of Lyman-α images detected in each field with a redshift confidence of 2 or 3 and a Lyman-α line with S/N > 3. The boldface values are the number of unique LAEs detected in each cluster with high redshift confidence. The last columns indicates the effective volume surveyed (Veff) at 2.9 < z < 6.7 with MUSE for Lyman-α emitters, for a magnification of the brightest image higher than 1.5 and 5.4, respectively.
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