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Table A.2.

Properties of galaxies in the control sample.

Name Cluster RA DEC z M* Mem JType fHαout LHαout T-type (vis) Comments References
[J2000] [J2000] [109 M] [1039erg/s/cm2]
A3128_B_0148 A3128 03:27:31.09 -52:59:07.7 0.057459 7.1±1.6 1 0.5 0 . 02 0.01 0.04 $ 0.02^{0.04}_{0.01} $ 3 . 2 1.4 6.7 $ 3.2^{6.7}_{1.4} $ 2 SF (14, 20, 27, 30, 32, 35, 36,
59, 61)
A3266_B_0257 A3266 04:27:52.58 -60:54:11.6 0.058359 8.3±1.8 1 1.0 0 . 18 0.17 0.20 $ 0.18^{0.20}_{0.17} $ 23 . 5 21.7 26.2 $ 23.5^{26.2}_{21.7} $ 3.3 SF (14, 20, 27, 30, 32, 35, 36,
59, 61)
A3376_B_0261 A3376 06:00:13.68 -39:34:49.2 0.050596 34.0±6.5 1 0.0 2.5 SF (14, 20, 27, 30, 32, 35, 36,
59, 60, 61)
A970_B_0338 A970 10:19:01.65 -10:10:36.9 0.059026 11.6±2.1 1 0.5 0 . 01 0.03 0.0 $ 0.01^{0.0}_{0.03} $ 2 . 2 0.5 5.4 $ 2.2^{5.4}_{0.5} $ 4.3 SF (14, 20, 27, 30, 32, 35, 36,
59, 61)
A1069_B_0103 A1069 10:39:36.49 -08:56:34.8 0.063479 21.5±3.6 1 4.0 -1.2 k (24)
A3128_B_0248 A3128 03:29:23.42 -52:26:02.9 0.053022 19.7±2.4 1 4.0 -2.3 k+a (24)
A3158_11_91 A3158 03:41:16.75 -53:24:00.6 0.061346 12.9±2.0 1 4.0 2.3 a+k (24)
A3158_B_0223 A3158 03:41:59.80 -53:28:04.2 0.056209 20.4±2.4 1 4.0 1.1 k (24)
A3158_B_0234 A3158 03:42:24.68 -53:29:26.0 0.066023 7.2±1.2 1 4.0 1.0 a+k (24)
A3376_B_0214 A3376 06:00:43.18 -39:56:41.6 0.047285 5.4±1.1 1 4.0 1.2 k+a (24)
A500_22_184 A500 04:38:46.41 -22:13:22.4 0.072477 3.6±0.5 1 4.0 -1.9 a+k (24)
A500_F_0152 A500 04:38:21.25 -22:13:02.2 0.069506 1.5±0.4 1 4.0 2.7 a+k (24)

Notes. Columns include the following: Galaxy ID, hosting cluster, coordinates, spectroscopic redshift, stellar mass, membership, JType, fraction and total luminosity of Hα emission outside the galaxy disk, morphological type, star forming classification, and references to the papers in which the galaxy is discussed. Hubble types are 6=Scd, 5=Sc, 4=Sbc, 3=Sb, 2=Sab, 1=Sa, 0=S0/a, -1=S0+, -2=S0, -4=E/S0, and -5=E.

References. (14) Vulcani et al. (2018a), (20) Vulcani et al. (2019a), (24) Vulcani et al. (2020a), (27) Franchetto et al. (2020), (30) Vulcani et al. (2020b), (32) Tomičić et al. (2021a), (35) Tomičić et al. (2021b), (36) Franchetto et al. (2021b), (59) Marasco et al. (2023), (60) Moretti et al. (2023), (61) Peluso et al. (2023).

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