The VISCACHA survey - XIV. Chemical evolution history of the SMC: The Southern Bridge Clusters

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Volume 701 (September 2025)

A&A, 701 (2025) A222

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Table A.1.

Literature parameters for our cluster sample.

Cluster	[Fe/H]	Age	E(B-V)	d	Reference
		(Gyr)	(mag)	(kpc)
B 91	–	0.796 ± 0.46	0.24 ± 0.10	–	Rafelski & Zaritsky (2005)
	–	0.794	0.12	–	Glatt et al. (2010)

B 98ne	–	1.40 $_{- 0.35}^{+ 5.77}$ $^{+5.77}_{-0.35}$	–	–	Rafelski & Zaritsky (2005)
	-0.96±0.05	3.50±0.50	0.09±0.04	55.20±2.50	Parisi et al. (2024)

BS 75	–	1.26	0.05	–	Glatt et al. (2010)
	–	1.78	0.00	–	Maia et al. (2014)
	-0.48±0.26	2.51	0.03±0.01	59.70	Perren et al. (2017)
	-0.99±0.10	2.40±0.20	0.10±0.04	60.5±2.50	Parisi et al. (2024)

BS 80	–	1.00	0.02	–	Glatt et al. (2010)
	-0.88±0.65	3.98	0.020±0.009	64.27	Perren et al. (2017)
	-1.00±0.08	3.00±0.50	0.08±0.04	58.9±3.30	Parisi et al. (2024)

HW 20	–	5.69 $_{- 0.41}^{+ 4.32}$ $^{+4.32}_{-0.41}$	–	–	Rafelski & Zaritsky (2005)
	-0.55 $_{- 0.10}^{+ 0.13}$ $^{+0.13}_{-0.10}$	1.10 $_{- 0.14}^{+ 0.08}$ $^{+0.08}_{-0.14}$	0.07 $_{- 0.01}^{+ 0.02}$ $^{+0.02}_{-0.01}$	62.20 $_{- 1.20}^{+ 2.50}$ $^{+2.50}_{-1.20}$	Maia et al. (2019)

HW 27	–	0.104	–	–	Rafelski & Zaritsky (2005)
	–	0.199	0.05	–	Glatt et al. (2010)

HW 31	–	1.26	0.57±0.4	–	Rafelski & Zaritsky (2005)
	–	4.60±0.20	–	–	Parisi et al. (2014)
	-0.40±0.22	3.16±0.05	0.05±0.10	61.36±0.80	Perren et al. (2017)
	-0.89±0.04	–	–	–	De Bortoli et al. (2022)
	-0.90±0.05	4.57±0.63	–	54.95±2.50	Illesca et al. (2025)

HW 36		1.38 $_{- 0.03}^{+ 4.90}$ $^{+4.90}_{-0.03}$	–	–	Rafelski & Zaritsky (2005)
	–	1.32 $_{- 0.30}^{+ 0.72}$ $^{+0.72}_{-0.30}$	0.09	–	Gatto et al. (2021)
	-0.84±0.14	2.80±0.70	0.05±0.06	58.1±4.30	Parisi et al. (2024)

HW 38	–	∼0.60	0.67±0.18	–	Rafelski & Zaritsky (2005), Glatt et al. (2010)
	-0.85	3.89 $_{- 1.90}^{+ 0.27}$ $^{+0.27}_{-1.90}$	0.06	–	Gatto et al. (2021)

HW 44	-0.6	0.42 ± 0.35	0.11	–	Gatto et al. (2021)

HW 47	-0.92±0.04	3.30±0.50	–	–	Parisi et al. (2009, 2014)
	-0.40±0.22	1.58±0.10	0.02±0.007	61.9±0.62	Perren et al. (2017)
	-0.90±0.02	2.51±0.15	–	54.95±1.50	Illesca et al. (2025)

HW 66	-1.30/-1.35±0.20	4.00±0.90/3.50±1.00	0.05	–	Piatti (2011)
	–	3.40±0.40	–	–	Parisi et al. (2014)
	-0.88±0.65	2.82	0.02±0.01	64.27	Perren et al. (2017)
	-1.16±0.04	4.00±0.50	0.16±0.04	57.50±2.40	Parisi et al. (2024)

K 37	–	1.00	–	–	Rafelski & Zaritsky (2005)
	−0.79 ± 0.11	1.80 ± 0.20	–	–	Parisi et al. (2015, 2014)
	−0.58 ± 0.33	1.12 ± 0.07	0.04 ± 0.01	62.52 ± 1.3	Perren et al. (2017)
	-0.81 $_{- 0.14}^{+ 0.13}$ $^{+0.13}_{-0.14}$	1.81 $_{- 0.21}^{+ 0.24}$ $^{+0.24}_{-0.21}$	0.05 $_{- 0.02}^{+ 0.01}$ $^{+0.01}_{-0.02}$	62.40 $_{- 1.80}^{+ 2.30}$ $^{+2.30}_{-1.80}$	Maia et al. (2019)
	-0.80±0.01	1.77±0.08	–	53.46±0.97	Illesca et al. (2025)

K 44		5.64	0.78±0.04	–	Rafelski & Zaritsky (2005)
	-0.85±0.04	–	–	–	Parisi et al. (2015)
	-0.85	3.71±0.07	0.09	–	Gatto et al. (2021)
	-0.78±0.03	–	–	–	Parisi et al. (2022)

L 106	-0.88±0.06	2.00±0.30	–	–	Parisi et al. (2009, 2014)
	-0.70±0.43	1.58±0.10	0.00±0.01	59.2±0.06	Perren et al. (2017)

L 112	-1.08±0.07	5.10±0.30	–	–	Parisi et al. (2014, 2015)
	-0.88±0.65	3.98±0.10	0.01±0.01	63.09±1.40	Perren et al. (2017)

L 116	-1.10±0.02	2.80±1.00	0.06	–	Piatti et al. (2001)
	-0.89±0.02	–	–	–	Parisi et al. (2022)
	-1.14±0.08	2.45±0.28	–	42.27±3.27	Illesca et al. (2025)

RZ 107	–	1.37 $_{- 0.01}^{+ 2.08}$ $^{+2.08}_{-0.01}$	–	–	Rafelski & Zaritsky (2005)
	-0.83±0.10	2.90±0.20	0.06±0.04	67.9±3.40	Parisi et al. (2024)

RZ 158	–	7.27 $_{- 0.18}^{+ 2.73}$ $^{+2.73}_{-0.18}$	–	–	Rafelski & Zaritsky (2005)
	-0.90 $_{- 0.39}^{+ 0.43}$ $^{+0.43}_{-0.39}$	4.80 $_{- 1.30}^{+ 1.60}$ $^{+1.60}_{-1.30}$	0.06	54.70±3.5	Bica et al. (2022)
	-1.11±0.05	4.70±1.40	0.08±0.05	56.00±4.40	Parisi et al. (2024)

NGC 643	–	1.50±0.30	–	–	Bica et al. (1986)
	-0.82±0.03	2.00±0.30	–	–	Parisi et al. (2009, 2014)

SB clusters already studied, but not in our sample

HW 79	-1.30/-1.40±0.2	5.00±1.30/4.30±1.20	0.06/0.07	–	Piatti (2011)
	–	4.10±0.50	–	–	Parisi et al. (2014)
	-0.88±0.65	6.31	0.01±0.01	63.68	Perren et al. (2017)
	-1.26±0.03	4.9±0.20	0.08±0.02	56.5±1.1	Parisi et al. (2024)

NGC 339	-1.19±0.10	–	–	–	Da Costa & Hatzidimitriou (1998)
	–	6.5±0.50	0.06/0.04	56.2	Glatt et al. (2008)
	-1.10±0.12	5.6±0.08	0.04	–	Narloch et al. (2021)
	-1.24±0.01	–	–	–	Mucciarelli et al. (2023)

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