The MUSE view of ram pressure stripped galaxies in clusters: The GASP sample

Open Access

Table A.1.

Continued.

Name	Cluster	RA	DEC	z	M_*	Mem	JType	f_Hα^out	L_Hα^out	T-type	References
		[J2000]	[J2000]		[10⁹ M_⊙]				[10³⁹erg/s/cm²]
JO41	A1631a	12:53:54.79	-15:47:20.1	0.047729	16.0±2.5	1	0.5	$0 . 05_{0.02}^{0.11}$ $0.05^{0.11}_{0.02}$	$3 . 65_{1.3}^{8.3}$ $3.65^{8.3}_{1.3}$	3.7	(14, 20, 21, 27, 30, 32, 35, 36, 41, 59, 61, 65,
											69)
JO45	A168	01:13:16.58	+00:12:05.8	0.042559	1.5±0.3	1	0.5	$0 . 04_{0.06}^{0.02}$ $0.04^{0.02}_{0.06}$	$7 . 5_{2.6}^{17.3}$ $7.5^{17.3}_{2.6}$	4.8	(14, 20, 21, 27, 30, 32, 35, 36, 41, 59, 61, 65,
											69)
JO47	A168	01:15:57.67	+00:41:36.0	0.04274	4.0±0.6	1	1.0	$0 . 08_{0.04}^{0.12}$ $0.08^{0.12}_{0.04}$	$7 . 01_{3.83}^{11.5}$ $7.01^{11.5}_{3.83}$	3.9	(14, 21, 27, 29, 30, 32, 35, 36, 41, 59, 61, 65,
											69)
JO49	A168	01:14:43.85	+00:17:10.1	0.045125	47.4±6.5	1	1.0	$0 . 02_{0.01}^{0.03}$ $0.02^{0.03}_{0.01}$	$6 . 66_{4.1}^{10.3}$ $6.66^{10.3}_{4.1}$	4.4	(13, 14, 21, 27, 29, 30, 32, 35, 36, 41, 43, 59,
											60, 61, 65, 69)
JO5	A1069	10:41:20.38	-08:53:45.6	0.064783	18.7±4.4	1	0.3	$0 . 02_{0.04}^{0.02}$ $0.02^{0.02}_{0.04}$	–	3.7	(14, 20, 21, 27, 30, 32, 35, 36, 59, 61, 65, 69)
JO60	A1991	14:53:51.57	+18:39:06.4	0.062187	25.1±6.5	1	2.0	$0 . 08_{0.07}^{0.09}$ $0.08^{0.09}_{0.07}$	$58 . 4_{53.0}^{65.0}$ $58.4^{65.0}_{53.0}$	5.0	(13, 14, 21, 27, 30, 32, 35, 36, 41, 43, 47, 57,
											59, 60, 61, 65, 66, 69)
JO68	A2399	21:56:22.00	-07:54:29.0	0.056117	9.9±2.1	1	0.3	$0 . 01_{0.003}^{0.04}$ $0.01^{0.04}_{0.003}$	$2 . 2_{0.4}^{6.3}$ $2.2^{6.3}_{0.4}$	5.0	(14, 20, 21, 27, 30, 32, 35, 36, 59, 61, 65, 69)
JO69	A2399	21:57:19.20	-07:46:43.8	0.054984	8.0±2.1	1	1.0	$0 . 04_{0.03}^{0.05}$ $0.04^{0.05}_{0.03}$	$11 . 4_{8.8}^{14.8}$ $11.4^{14.8}_{8.8}$	5.2	(14, 21, 29, 30, 32, 35, 36, 41, 59, 61, 65, 69,
											70)
JO70	A2399	21:56:04.07	-07:19:38.0	0.057759	29.0±6.1	1	1.0	$0 . 05_{0.05}^{0.06}$ $0.05^{0.06}_{0.05}$	$28 . 3_{24.8}^{34.6}$ $28.3^{34.6}_{24.8}$	4.0	(14, 21, 27, 29, 30, 32, 35, 36, 41, 59, 61, 65,
											69, 70)
JO73	A2415	22:04:25.99	-05:14:47.0	0.071251	*10.6±2.6	0	1.0	$0 . 10_{0.09}^{0.12}$ $0.10^{0.12}_{0.09}$	$15 . 8_{13.5}^{19.1}$ $15.8^{19.1}_{13.5}$	4.1	(14, 20, 27, 30, 32, 35, 36, 61, 65, 69)
JO85	A2589	23:24:31.36	+16:52:05.3	0.035453	46.3±9.4	1	2.0	$0 . 16_{0.15}^{0.16}$ $0.16^{0.16}_{0.15}$	$151_{146}^{153}$ $151^{153}_{146}$	2.0	(14, 21, 27, 29, 30, 32, 35, 36, 41, 43, 59, 61,
											65, 69, 70)
JO89	A2593	23:26:00.60	+14:18:26.3	0.04235	5.3±1.0	1	0.5	$0 . 07_{0.02}^{0.07}$ $0.07^{0.07}_{0.02}$	$2 . 0_{0.5}^{6.1}$ $2.0^{6.1}_{0.5}$	5.5	(14, 20, 21, 27, 30, 32, 35, 36, 41, 59, 61, 65,
											69)
JO93	A2593	23:23:11.74	+14:54:05.0	0.036984	35.0±5.8	1	1.0	$0 . 11_{0.11}^{0.11}$ $0.11^{0.11}_{0.11}$	$49 . 1_{47.0}^{51.0}$ $49.1^{51.0}_{47.0}$	2.8	(14, 21, 27, 29, 32, 35, 36, 41, 59, 61, 65, 69,
											70)
JO95	A2657	23:44:26.66	+09:06:55.8	0.043322	2.3±0.4	1	1.0	$0 . 10_{0.08}^{0.13}$ $0.10^{0.13}_{0.08}$	$8 . 5_{6.8}^{12.0}$ $8.5^{12.0}_{6.8}$	5.0	(13, 14, 21, 27, 36, 41, 59, 61, 65)
JW10	A500	04:39:18.19	-21:57:49.6	0.07179	9.8±2.4	1	-9.0	$0 . 12_{0.11}^{0.14}$ $0.12^{0.14}_{0.11}$	$23 . 9_{21.5}^{26.8}$ $23.9^{26.8}_{21.5}$	5.2	(14, 21, 30, 32, 35, 36, 65)
JW100	A2626	23:36:25.06	+21:09:02.5	0.061891	293.2±70.2	1	2.0	$0 . 20_{0.20}^{0.20}$ $0.20^{0.20}_{0.20}$	$225_{223}^{227}$ $225^{227}_{223}$	1.4	(6, 13, 14, 19, 21, 22, 23, 27, 30, 31, 32, 35,
											36, 37, 38, 39, 40, 41, 43, 50, 51, 53, 56, 57,
											59, 61, 63, 65, 66, 67, 68, 69, 72)
JW105	A2717	00:03:00.49	-36:06:39.7	0.051505	*1.5±0.2	1	0	0.00	–	-4.3	(59, 65)
JW108	A3376	06:00:47.96	-39:55:07.4	0.047688	30.2±7.7	1	3.0	$0 . 03_{0.01}^{0.06}$ $0.03^{0.06}_{0.01}$	$1 . 86_{0.41}^{4.81}$ $1.86^{4.81}_{0.41}$	6.1	(14, 21, 30, 32, 35, 41, 59, 60, 61, 65, 66, 69)
JW115	A3497	12:00:47.95	-31:13:41.6	0.072485	5.3±1.4		1.0	$0 . 09_{0.05}^{0.14}$ $0.09^{0.14}_{0.05}$	$10 . 0_{5.3}^{17.2}$ $10.0^{17.2}_{5.3}$	2.8	(14, 21, 27, 30, 32, 35, 36, 41, 59, 61, 65, 69)
JW29	A1644	12:57:49.48	-17:39:57.1	0.043119	3.2±0.6	1	0.5	$0 . 06_{0.03}^{0.12}$ $0.06^{0.12}_{0.03}$	$5 . 86_{2.6}^{13.2}$ $5.86^{13.2}_{2.6}$	6.1	(14, 21, 30, 32, 35, 36, 41, 59, 61, 65, 69)
JW36	A1644	12:56:44.22	-17:39:48.6	0.050062	0.5±0.1	1	4.0	0.00	–	5.2	(59, 65)
JW39	A1668	13:04:07.71	+19:12:38.5	0.066319	161.4±28.5	1	2.0	$0 . 14_{0.14}^{0.14}$ $0.14^{0.14}_{0.14}$	$125_{120}^{129}$ $125^{129}_{120}$	3.5	(13, 14, 21, 27, 29, 30, 32, 35, 36, 40, 41, 43,
											47, 50, 51, 56, 57, 59, 61, 63, 65, 66, 67, 68,
											69)
JW56	A1736	13:27:03.03	-27:12:58.2	0.038664	1.1±0.3	1	2.0	$0 . 33_{0.30}^{0.38}$ $0.33^{0.38}_{0.30}$	$14 . 1_{12.0}^{17.2}$ $14.1^{17.2}_{12.0}$	3.0	(14, 21, 27, 29, 30, 32, 35, 36, 41, 59, 61, 65,
											67, 69, 70)

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, 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. Stellar mass is computed within the galaxy disk defined in Sect. 2, except for galaxies with an asterisks, for which the galaxy disk was not measured, as the irregularities of the galaxy and the disk is defined as 1σ above the background level on a 2D image of the near-Hα continuum.

References. (1) Poggianti et al. (2017b), (2) Bellhouse et al. (2017), (3) Fritz et al. (2017), (4) Gullieuszik et al. (2017), (5) Moretti et al. (2018b), (6) Poggianti et al. (2017a), (9) Jaffé et al. (2018), (10) Moretti et al. (2018a), (11) George et al. (2018), (13) Poggianti et al. (2019a), (14) Vulcani et al. (2018a), (15) Bellhouse et al. (2019), (17) Ramatsoku et al. (2019), (18) George et al. (2019), (19) Radovich et al. (2019), (20) Vulcani et al. (2019a), (21) Gullieuszik et al. (2020), (22) Moretti et al. (2020b), (23) Poggianti et al. (2019b), (25) Deb et al. (2020), (26) Ramatsoku et al. (2020), (27) Franchetto et al. (2020), (28) Müller et al. (2021), (29) Bellhouse et al. (2021), (30) Vulcani et al. (2020b), (31) Moretti et al. (2020a), (32) Tomičić et al. (2021a), (33) Vulcani et al. (2021), (34) Campitiello et al. (2021), (35) Tomičić et al. (2021b), (36) Franchetto et al. (2021b), (37) Luber et al. (2022), (38) Ignesti et al. (2022b), (39) Deb et al. (2022), (40) Franchetto et al. (2021a), (41) Peluso et al. (2022), (43) Ignesti et al. (2022a), (44) Bartolini et al. (2022), (45) Sánchez-García et al. (2023), (48) George et al. (2023), (50) Giunchi et al. (2023a), (51) Gullieuszik et al. (2023), (53) Bacchini et al. (2023), (56) Giunchi et al. (2023b), (57) Tomičić et al. (2024), (58) Ignesti et al. (2023a), (59) Marasco et al. (2023), (60) Moretti et al. (2023), (61) Peluso et al. (2023), (63) Werle et al. (2024), (65) Salinas et al. (2024) (66) George et al. (2024), (67) Ignesti et al. (2024), (68) Giunchi et al. (2025), (69) Peluso et al. (2025), (70) George et al. (2025), (71) Merluzzi et al. (2013), (72) Sun et al. (2021).

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