The GALAH survey: Improving chemical abundances using star clusters

Open Access

Table A.2

Globular clusters used in this work.

Cluster	N_GALAH		age^§	metallicity	notes
	all	no flag	[Gyr]	[Fe/H]
47 Tuc	568	417	13.4	-0.74*	1
E 3	16	5	12.8	-0.89^∥
NGC 288	107	58	10.6	-1.27*	1
NGC 362	52	47	10.4	-1.11*	1
NGC 1261	32	10	10.2	-1.37**
NGC 1851	20	13	9.6	-1.13*	1
NGC 2808	53	42	10.9	-1.07*
NGC 3201	62	1	10.2	-1.39*
NGC 5904	86	54	10.6	-1.21*
NGC 6121	295	226	12.5	-1.07*	1
NGC 6254	14	11	11.4	-1.51*
NGC 6362	12	5	13.7	-1.07^†
NGC 6397	195	91	12.7	-2.02*	1
NGC 6544	78	51	11.8^¶	-1.52*	1
NGC 6656	238	186	12.7	-1.70*	1
NGC 6752	123	99	11.8	-1.47*
NGC 6809	63	62	12.3	-1.76*
NGC 7089	12	0	11.8	-1.47*	1
NGC 7099	24	23	12.9	-2.29^‡	1
ω Cen	264	247	11.4	-1.60*

1: Cluster was used for calculating trends (giants)

* Schiavon et al. (2024)

^†Massari et al. (2017)

^‡O’Malley & Chaboyer (2018)

^§Marín-Franch et al. (2009)

^¶Cabrera-Ziri & Conroy (2022)

^∥Monaco et al. (2018)

**Muñoz et al. (2021)

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