Open Access

Table A.2

Literature comparisons for the degree of rotation in each cluster.

Cluster L10 B12 F14 L15 K15 K18 F18 G18 B18 V19 S19 M23 P24 This work
NGC 104
NGC 288 X X X X X X X
NGC 1261 X X
NGC 1851 X X X
NGC 2808 X X X
NGC 3201 X
NGC 4590 X X X X X X
NGC 4833 X X X X
NGC 5024 X X X
NGC 5053 X
NGC 5272 X (✓)
NGC 5286 X X
NGC 5904
NGC 5986 X
NGC 6101
NGC 6121 X X
NGC 6205 X
NGC 6218 X X X X X (✓) X
NGC 6254 X X X
NGC 6341 X (✓)
NGC 6366 X X X
NGC 6656 X
NGC 6752 X X X X (✓)
NGC 6809 (✓)
NGC 6838 X X X X X
NGC 6934 X
NGC 6981
NGC 7078
NGC 7089
NGC 7099 X X X X (✓)

Notes. The detection of rotation from literature in comparison to this work (following the style of Table 3 of Sollima et al. (2019)) in which checkmarks, crosses and tildes indicate positive, negative and 2σ detections, respectively. Clusters in our sample for which rotation could not be analysed due to a low number of LOS measurements are marked with a dash. Each column corresponds to the previous works of Lane et al. (2010) (L10), Bellazzini et al. (2012) (B12), Fabricius et al. (2014) (F14), Lardo et al. (2015) (L15), Kimmig et al. (2015) (K15), Kamann et al. (2018) (K18), Ferraro et al. (2018) (F18), Gaia Collaboration (2018) (G18), Bianchini et al. (2018) (B18), Vasiliev (2019) (V19), Sollima et al. (2019) (S19), Martens et al. (2023) (M23), and Petralia et al. (2024) (P24). Checkmarks within parenthesis in the S19 column indicate GCs with uncertain detections in the work of Sollima et al. (2019) (see details within).

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