X-Shooting ULLYSES: Massive stars at low metallicity. XIV. Properties of SMC late-O and B supergiants reveal the metallicity dependence of winds in the Magellanic Clouds.

This repository contains complementary material to the publication "X-Shooting ULLYSES: Massive stars at low metallicity. XIV. Properties of SMC late-O and B supergiants reveal the metallicity dependence of winds in the Magellanic Clouds." by T. Alkousa, P.A. Crowther, J.M. Bestenlehner et al. 2025. The pdf file contains the following sections: Appendix G: Contains brief comments on the issues and quality of individual line fits of each star. Appendix H: Spectral energy distribution (SED) fits. Appendix I: Spectral fits of line diagnostics. Appendix J: Overall ultraviolet and optical spectral fits. The optical and ultraviolet data used in this study are drawn from the publicly available Data Release 1 (DR1) of the XShootU collaboration (for further information on the data, see Vink et al. 2023 A&A 675, A174 https://doi.org/10.1051/0004-6361/202245650 and Sana et al. 2024 A&A 688, A104 https://doi.org/10.1051/0004-6361/202347479)