Chemical abundances [X/Fe] as a function of [Fe/H] for the Sgr sample (filled blue dots) are compared with MW halo stars and members of various MW satellites. Specifically, data for the MW halo (empty gray dots) are queried from the SAGA database (Suda et al. 2008). The GES stars (orange) are taken from Carrillo et al. (2022), LMC members (pink) from Van der Swaelmen et al. (2013), and Na measurements from Pompéia et al. (2008). Finally, stars from the Fornax galaxy (purple) are from Letarte et al. (2010), while Sculptor members (green) are from Hill et al. (2019).