Averaged ⟨[Mg,Si,Ca,Ti/Fe]⟩ ratio for MW stars (black dots) and NGC 1261 (star symbols). The stellar component of Gaia-Enceladus (Helmi et al. 2018) is overlaid as 1, 2, and 3σ contours. A sample of reference GCs dynamically associated with Gaia-Enceladus, color-coded by their Galactocentric distance, are shown. The GC abundances from the literature are from Francois (1991), McWilliam et al. (1992), Shetrone & Keane (2000), Cohen & Melendez (2005), Carretta et al. (2011, 2013), Roederer & Sneden (2011), Kacharov et al. (2013), Lovisi et al. (2013), Khamidullina et al. (2014), Koch & McWilliam (2014), Yong et al. (2014), Roederer & Thompson (2015), Johnson et al. (2017), Marino et al. (2017), and Koch et al. (2019b).