Metallicities and ages for 35 star clusters and their surrounding fields in the Small Magellanic Cloud

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Volume 647 (March 2021)

A&A, 647 (2021) A135

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Table 5.

Reddenings, metallicities and ages of star clusters from the literature.

Name	E(B − V)	[Fe/H]	Age	log(Age)
	(mag)	(dex)	(Gyr)	(yr)
Lindsay 113	0.00 ± 0.02⁵, 0.03 ± 0.01^{11, 15, 23}	−1.37 ± 0.16⁴, −1.44 ± 0.16⁴	6.0 ± 1.0⁴, 4.0 ± 0.7⁵	9.55 ± 0.05²³, 9.65³⁰
	0.047¹⁶, 0.04²⁶, 0.02²⁷, 0.01²⁸	−1.12 ± 0.12⁴, −1.17 ± 0.12⁴	5.3 ± 1.3⁵, 5.3 ± 1.0¹¹
	0.0^22a, 0.077^32b	−1.24 ± 0.11⁴, −1.40 ± 0.25¹¹	4.0 ± 0.4²⁰, 4.6 ± 1.0²⁶
		−1.7 ± 0.3²⁰, −1.3 ± 0.3²⁰	4.5 ± 0.5^27, 28
		−0.88 ± 0.065²³, −1.19 ± 0.03²⁶
		−1.4²⁷, −1.3²⁸, −1.03³⁰

NGC 339	0.03^{1, 14, 27}, 0.03 ± 0.04⁵, 0.032¹²	−1.5 ± 0.2¹, −1.36 ± 0.1⁴	> 10¹, 4.0 ± 1.5⁴, 5.0 ± 0.6⁵	9.8 ± 0.09¹⁹, 9.78³⁰
	0.04 ± 0.01¹⁹, 0.020 ± 0.007²³	−1.46 ± 0.1⁴, −1.12 ± 0.1⁴	6.3 ± 1.3⁵, 6.6¹⁴, 6.0 ± 0.5¹⁸
	0.02²⁶, 0.054^32b	−1.19 ± 0.12^4, 30, −1.5 ± 0.14⁵	5.4 ± 1.0¹⁹
		−1.18¹⁴, −1.3 ± 0.25¹⁹
		−0.88 ± 0.065²³, −1.27 ± 0.03²⁶

NGC 361	0.03^1, 26, 0.07 ± 0.03^5, 14	−1.25 ± 0.20¹, −1.45 ± 0.11^{5, 14, 30}	8.0 ± 1.5¹, 6.8 ± 0.5⁵	9.91³⁰
	0.037¹⁶, 0.0²², 0.083³¹, 0.102^32b	−1.08 ± 0.10^14, 26, −0.9 ± 0.2¹⁵	8.1 ± 1.2⁵, 5.6¹⁴, 6.8 ± 0.5¹⁶
		−0.8 ± 0.3²⁰, −0.7 ± 0.3²⁰	2.0 ± 0.4²⁰
		−1.13 ± 0.03²⁶

Lindsay 1	0.06 ± 0.02⁵, 0.02^12, 27, 0.04²⁶	−1.14 ± 0.10^{1, 12, 27}, −1.17 ± 0.10¹	10.0 ± 2.0¹, 7.7 ± 0.4⁵	9.88³⁰
	0.044^32b	−0.99 ± 0.11¹, −1.01 ± 0.11^1, 14	9.0 ± 1.0⁵, 8.3 ± 0.7¹²
		−1.35 ± 0.08⁵, −1.10 ± 0.10⁵	7.7 ± 0.7¹², 7.5 ± 0.5^{12, 18, 26, 27}
		−1.11 ± 0.02²⁶, −1.04 ± 0.03³⁰

Lindsay 6	0.03¹⁹, 0.020 ± 0.006²³	−0.9 ± 0.2¹⁹, −1.24 ± 0.03^22, 30	3.3 ± 0.7¹⁹, 7.0²², 7.08²²	9.75 ± 0.07²³, 9.73³⁰
	0.095^22b, 0.063³¹, 0.044^32b	−0.88 ± 0.065²³

NGC 330	0.03^3, 29, 0.06³, 0.10^8, 17	−1.26³, −1.17³, −0.93 ± 0.16³	0.04 ± 0.4²⁰, 0.04²⁴	7.5 ± 0.1⁸, 8.0⁹, 7.4¹⁷
	0.11²⁴, 0.05^20a, 0.08^9b	−0.69 ± 0.11⁷, −0.94 ± 0.02⁶		7.63³⁰
	0.095³¹, 0.072^32b	−1.0 ± 0.1², −0.5 ± 0.3²⁰,
		−1.0 ± 0.3²⁰, −0.90²⁴, −1.15 ± 0.06²⁹,
		−0.82 ± 0.10³⁰

OGLE-CL SMC 45	0.07⁸, 0.02¹³, 0.10¹⁷, 0.03²⁹	−0.7¹², −0.01 ± 0.09^23, 30	0.22¹³	8.4 ± 0.1^8, 9, 8.35¹⁷, 8.38³⁰
	0.10 ± 0.04²³, 0.08^9b, 0.077³¹, 0.064^32b	−0.85 ± 0.15²⁹		6.9 ± 0.07²³

Lindsay 27	0.06⁸, 0.11^15, 19, 0.00 ± 0.03²³	−1.3 ± 0.3¹⁹, −1.14 ± 0.06^22, 30	2.1 ± 0.3¹¹, 6.3 ± 1.0²²	> 9⁸, 9.45 ± 0.06²³, 9.66³⁰
	0.084³¹, 0.067^32b	−0.88 ± 0.065²³	4.6 ± 0.6²²

Lindsay 19	0.10⁸, 0.02^15, 19, 0.04^9b, 23	−0.75 ± 0.20¹¹, −0.87 ± 0.03^22, 30	2.1 ± 0.3^11, 19	> 9⁸, 8.9⁹, 9.45 ± 0.08²³
	0.16^25b, 0.079³¹, 0.058^32b	−0.88 ± 0.065²³		8.5²⁵, 9.6³⁰

NGC 265	0.11⁸, 0.05¹¹, 0.09¹⁷	−0.62⁹, −0.6 – −1.1¹¹	0.25 ± 0.12¹¹	8.0±0.1⁸, 8.4⁹, 8.5 ± 0.3¹⁰
	0.04 ± 0.02²³, 0.08^9b, 0.17^25b	−0.28 ± 0.16^23, 30		8.7 ± 0.2¹⁰, 8.35¹⁷, 8.25^25, 30
	0.077³¹, 0.095^32b			8.45 ± 0.06²³

NGC 376	0.07⁸, 0.14¹¹, 0.08¹⁷, 0.03²⁹	−0.5 ± 0.3²⁰, −0.40 ± 0.29^23, 30	0.025 ± 0.01¹¹, 0.028²⁹	7.5 ± 0.1^8, 17, 7.2⁹, 7.8²³
	0.00 ± 0.02²³, 0.4²⁰, 0.08^9b	−0.55 ± 0.09²⁹	0.03 ± 0.4²⁰	7.35²⁵, 7.4³⁰
	0.15^25b, 0.090³¹, 0.059^32b

IC 1611	0.08⁸, 0.15¹¹, 0.05¹⁷, 0.03²⁹	−0.7²⁹, −0.80 ± 0.09²⁹	0.10 ± 0.04²⁹	8.2 ± 0.1^8, 17, 8.1⁹, 8.15²⁵
	0.08^9b, 0.06^25b, 0.110³¹, 0.079^32b

IC 1612	0.07⁸, 0.08^9b, 0.06¹³, 0.13¹⁷	−0.7¹³, −0.10 ± 0.11^23, 30		7.7 ± 0.2⁸, 8.0^9, 17, 8.09¹³
	0.05 ± 0.01²³, 0.21^25b, 0.110³¹, 0.079^32b		–	8.10 ± 0.05²³, 7.47²⁵, 7.90³⁰
	0.079^32b

OGLE-CL SMC 32	0.1⁸, 0.05¹¹, 0.2¹⁷	−0.10 ± 0.18^23, 30	0.16 ± 0.07¹¹	8.0 ± 0.1⁸, 8.0^9, 23, 7.8^17, 25
	0.06 ± 0.03²³, 0.2^9b, 0.26^25b			7.93³⁰
	0.103³¹, 0.083^32b

Bruck 39	0.08^9b, 0.08¹⁷, 0.02 ± 0.04²³	−0.58 ± 0.54^23, 30	–	8.6 ± 0.2⁹, 8.65¹⁷, 8.9²³, 8.3²⁵
	0.20^25b, 0.103³¹, 0.083^32b			9.08³⁰

OGLE-CL SMC 68	0.09⁸, 0.25¹⁷, 0.16^9b, 0.077³¹	–	–	7.7 ± 0.2⁸, 7.0⁹, 7.4¹⁷
	0.057^32b			7.37³⁰

OGLE-CL SMC 69	0.08⁸, 0.1¹⁷, 0.2^9b, 0.3^25b	−0.75¹⁰	–	7.6 ± 0.1⁸, 7.0⁹,
	0.088³¹, 0.080^32b			7.8 ± 0.5¹⁰, 8.0 ± 0.3¹⁰,
				7.6¹⁷, 7.63²⁵, 7.4³⁰

OGLE-CL SMC 99	0.08⁸, 0.05¹⁷, 0.08^9b	–	–	7.6 ± 0.2⁸, 7.3⁹, 7.5¹⁷
	0.11^25b, 0.069³¹, 0.045^32b			7.7²⁵, 7.47³⁰

OGLE-CL SMC 129	0.09⁸, 0.05¹⁷, 0.12^9b	–	–	7.3 ± 0.1⁸, 7.3⁹, 7.4¹⁷
	0.098³¹, 0.105^32b			7.33³⁰

OGLE-CL SMC 142	0.06⁸, 0.08¹⁷, 0.14^9b, 0.13^25b	–	–	7.3 ± 0.1⁸, 6.9⁹, 7.0¹⁷
	0.078³¹, 0.082^32b			7.24²⁵, 7.07³⁰

[BS95] 123	0.08^9b, 0.07¹⁷, 0.11^25b, 0.078³¹	–	–	7.5⁹, 7.6¹⁷, 7.95²⁵, 7.55³⁰
	0.082^32b

OGLE-CL SMC 144	0.05⁸, 0.10^9b, 0.05¹⁷, 0.078³¹	–	–	7.6^8, 9, 7.7¹⁷, 7.67³⁰
	0.082^32b

OGLE-CL SMC 49	0.06⁸, 0.02¹⁷, 0.06 ± 0.03²³	−0.10 ± 0.14^23, 30	–	7.0 ± 0.2⁸, 8.0⁹, 7.9¹⁷
	0.08^9b, 0.086³¹, 0.058^32b			7.5 ± 0.3²³, 7.7³⁰

OGLE-CL SMC 50	0.12⁸, 0.16¹⁷, 0.15^9b	–	–	8.1 ± 0.1⁸, 7.9⁹, 8.2¹⁷
	0.11³¹, 0.197^32b			8.0³⁰

OGLE-CL SMC 54	0.10⁸, 0.08¹⁷, 0.05²¹, 0.04 ± 0.03²³	−0.01 ± 0.09^23, 30	–	8.0 ± 0.1⁸, 8.0^9, 17, 8.01³⁰
	0.08^9b, 0.13^25b, 0.079³¹, 0.048^32b			7.0 ± 0.4²³, 8.25²⁵

OGLE-CL SMC 61	0.12⁸, 0.15^9b, 0.104³¹, 0.081^32b	–	–	7.4 ± 0.2⁸, 7.8⁹, 7.6³⁰

OGLE-CL SMC 71	0.07⁸, 0.06¹⁷, 0.2^9b, 0.34^25b	–	–	7.5 ± 0.1⁸, 7.1⁹, 8.75¹⁷
	0.087³¹, 0.049^32b			7.88²⁵, 8.2³⁰

OGLE-CL SMC 205	0.08^9b, 17, 0.087³¹, 0.049^32b	–	–	8.1⁹, 8.3¹⁷, 8.2³⁰

OGLE-CL SMC 78	0.08^8, 17, 0.08^9b, 0.074³¹	–	–	7.9 ± 0.1⁸, 7.0⁹, 7.8¹⁷
	0.025^32b			7.57³⁰

OGLE-CL SMC 82	0.10^8, 17, 0.15^9b, 0.085³¹	–	–	7.8 ± 0.3⁸, 7.9^9, 17, 7.87³⁰
	0.038^32b

OGLE-CL SMC 88	0.20^9b, 0.085³¹, 0.038^32b	–	–	7.2^9, 30

OGLE-CL SMC 126	0.07⁸, 0.02¹⁷, 0.08^9b	–	–	8.0 ± 0.1⁸, 8.0⁹, 8.2¹⁷
	0.17^25b, 0.083³¹, 0.057^32b			7.89²⁵, 8.07³⁰

OGLE-CL SMC 128	0.09⁸, 0.07¹⁷, 0.08^9b	–	–	7.1 ± 0.3⁸, 7.3⁹, 8.0¹⁷
	0.099³¹, 0.098^32b			7.2³⁰
OGLE-CL SMC 143	0.09⁸, 0.2^9b, 0.093³¹, 0.113^32b	–	–	8.2 ± 0.2⁸, 7.5⁹, 7.85³⁰

OGLE-CL SMC 156	0.09⁸, 0.10¹⁷, 0.00^20a, 0.08^9b	−1.0 ± 0.3²⁰, −0.7 ± 0.3²⁰	0.2 ± 0.4²⁰	8.2 ± 0.1⁸, 8.1^{9, 17, 23}
	0.2^25b, 0.088³¹, 0.064^32b			7.8²⁵

Notes. ^(a)E(b − y). ^(b)E(V − I).

References. (1) Bica et al. (1986) (DDO, Hβ photometry); (2) Spite et al. (1991) (high-resolution spectroscopy); (3) Grebel & Richtler (1992) (Strömgren photometry); (4) Da Costa & Hatzidimitriou (1998) (low-resolution spectroscopy, CaT); (5) Mighell et al. (1998) (HST photometry, RGB slope); (6) Gonzalez & Wallerstein (1999) (high-resolution spectroscopy); (7) Hill (1997) (high-resolution spectroscopy); (8) Pietrzyński & Udalski (1999) (optical photometry); (9) Chiosi et al. (2006) (optical photometry); (10) Chiosi & Vallenari (2007) (HST photometry); (11) Piatti et al. (2007a,b) (Washington photometry); (12) Glatt et al. (2008) (HST photometry); (13) Piatti et al. (2008) (Washington photometry); (14) Mucciarelli et al. (2009) (NIR photometry, RGB slope); (15) Kučinskas et al. (2009) (NIR photometry, RGB slope); (16) Dias et al. (2010) (integrated spectroscopy); (17) Glatt et al. (2010) (optical photometry); (18) Glatt et al. (2011) (HST photometry); (19) Piatti (2011) (Washington photometry); (20) Livanou et al. (2013) (Strömgren photometry); (21) Maia et al. (2014) (Washington photometry); (22) Parisi et al. (2014) (low-resolution spectroscopy, CaT); (23) Perren et al. (2017) (Washington photometry, ASteCA); (24) Milone et al. (2018) (HST photometry); (25) Nayak et al. (2018) (optical photometry); (26) Piatti (2018) (Strömgren photometry); (27) Chantereau et al. (2019) (HST photometry); (28) Martocchia et al. (2019) (HST photometry); (29) Piatti et al. (2019) (Strömgren photometry); (30) Bica et al. (2020) (catalog); (31) Górski et al. (2020) (optical photometry); (32) Skowron et al. (2021) (optical photometry).

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