Table 1.
Properties of our targets.
| Galaxy | RA | Dec | zspec | M⋆ | SFR | sSFR | sSFRMS | K0 |
|---|---|---|---|---|---|---|---|---|
| (hh:mm:ss.s) | (dd:mm:ss.s) | (1011 M⊙) | (M⊙ yr−1) | (Gyr−1) | (Gyr−1) | (keV cm2) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| A209 | 01:31:52.53 | −13:36:40.5 | 0.206 | 2.00 ± 0.16 | < 0.12 (UV) | < 6.0 × 10−4 | 0.04 | 106 ± 27 |
| M0329 | 03:29:41.57 | −02:11:46.6 | 0.450 | 3.69 ± 0.21 | 42 ± 2 (UV) | 0.11 ± 0.01 | 0.07 | 11 ± 3 |
| 80 ± 21 (Hα) | 0.22 ± 0.06 | |||||||
| M0429 | 04:29:36.03 | −02:53:06.8 | 0.399 | 4.68 ± 0.23 | 28 ± 2 (UV) | 0.06 ± 0.01 | 0.06 | 17 ± 4 |
| 33 ± 9 (Hα) | 0.07 ± 0.02 | |||||||
| M0647 | 06:47:50.70 | +70:14:54.0 | 0.591 | 5.13 ± 1.79 | < 0.3 (UV) | < 5.8 × 10−4 | 0.10 | 225 ± 50 |
| M0744 | 07:44:52.80 | +39:27:26.5 | 0.686 | 8.20 ± 0.43 | 0.6 ± 0.1 (UV) | (7.3 ± 1.3)×10−4 | 0.11 | 42 ± 11 |
| A611 | 08:00:56.82 | +36:03:23.6 | 0.288 | 3.45 ± 0.42 | < 0.04 (UV) | < 1.2 × 10−4 | 0.04 | 125 ± 18 |
| M1115 | 11:15:51.90 | +01:29:55.0 | 0.352 | 2.19 ± 0.17 | 13 ± 1 (UV) | (5.5 ± 0.6)×10−2 | 0.07 | 15 ± 3 |
| 3.4 ± 1.0 (Hα) | (1.6 ± 0.5)×10−2 | |||||||
| A1423 | 11:57:17.36 | +33:36:39.7 | 0.213 | 1.96 ± 0.11 | 0.07 ± 0.03 (UV) | (3.6 ± 1.5)×10−4 | 0.04 | 68 ± 13 |
| M1206 | 12:06:12.17 | −08:48:02.9 | 0.440 | 4.93 ± 1.39 | 2.9 ± 0.6 (UV) | (5.9 ± 2.1)×10−3 | 0.06 | 69 ± 10 |
| CL1226 | 12:26:58.25 | +33:32:48.6 | 0.891 | 15.00 ± 1.99 | 0.9 ± 0.1 (UV) | (6.0 ± 1.0)×10−4 | 0.14 | 166 ± 45 |
| M1311 | 13:11:01.81 | −03:10:39.7 | 0.494 | 4.49 ± 1.05 | < 1.2 (UV) | < 2.7 × 10−3 | 0.08 | 47 ± 4 |
| RX1347 | 13:47:31.83 | −11:45:11.6 | 0.451 | 3.68 ± 0.85 | 22 ± 1 (UV) | (6.0 ± 1.4)×10−2 | 0.08 | 12 ± 20 |
| 12 ± 4 (Hα) | (3.3 ± 1.3)×10−2 | |||||||
| M1423 | 14:23:47.88 | +24:04:42.4 | 0.545 | 4.95 ± 0.13 | 27 ± 1 (UV) | (5.5 ± 0.2)×10−2 | 0.09 | 10 ± 5 |
| 33 ± 9 (Hα) | (6.7 ± 1.9)×10−2 | |||||||
| RX1532 | 15:32:53.79 | +30:20:59.5 | 0.361 | 2.20 ± 0.05 | 97 ± 4 (UV) | 0.44 ± 0.02 | 0.07 | 17 ± 2 |
| 140 ± 40 (Hα) | 0.64 ± 0.18 | |||||||
| M1720 | 17:20:16.75 | +35:36:26.2 | 0.391 | 3.83 ± 0.94 | 1.1 ± 0.2 (UV) | (2.9 ± 0.9)×10−3 | 0.06 | 24 ± 3 |
| 4.4 ± 1.2 (Hα) | (1.1 ± 0.4)×10−2 | |||||||
| A2261 | 17:22:27.20 | +32:07:56.9 | 0.224 | 1.74 ± 0.18 | < 0.06 (UV) | < 3.4 × 10−4 | 0.04 | 61 ± 8 |
| M1932 | 19:31:49.6 | −26:34:33.2 | 0.353 | 6.9 ± 0.8 | 280 ± 20 (UV) | 0.41 ± 0.06 | 0.04 | 14 ± 4 |
| 130 ± 40 (Hα) | 0.19 ± 0.06 | |||||||
| M2129 | 21:29:26.12 | −07:41:27.9 | 0.570 | 2.44 ± 0.17 | < 0.1 (UV) | < 4.1 × 10−4 | 0.13 | 200 ± 100 |
| RX2129 | 21:29:39.96 | +00:05:21.1 | 0.234 | 2.21 ± 0.32 | < 3 (UV) | < 0.01 | 0.04 | 21 ± 4 |
| < 49 (Hα) | < 0.22 |
Notes. (1) BCG name; (2–3) J2000 equatorial coordinates; (4) spectroscopic redshift; (5) stellar mass from Burke et al. (2015) except for M1932 (Cooke et al. 2016) ; (6) UV- and Hα-based SFR, corrected for dust extinction, from Fogarty et al. (2015), except for M0647 and M2129, for which the SFR upper limits are from Donahue et al. (2015); (7) specific SFR determined as sSFR = SFR/M⋆; (8) sSFR for main sequence field galaxies with redshift and stellar mass of our targets estimated using the relation found by Speagle et al. (2014); (9) central entropy 
of the cluster estimated by Donahue et al. (2015). Upper limits are at 3σ.
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