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Publication
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Work with us on data science and visualisation projects, and deploy your project as an app on top of Graph Search.
Context. Individual stars in dwarf spheroidal galaxies around the Milky Way Galaxy have been studied both photometrically and spectroscopically. Extremely metal-poor stars among them are very valuable because they should record the early enrichment in the Local Group. However, our understanding of these stars is very limited because detailed chemical abundance measurements are needed from high resolution spectroscopy.
Pascale Jablonka, Yves Revaz, Mahsa Sanati