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Abundances Working Group
Leads: Georges Kordopatis & Tadafumi Matsuno
Line detectability comparison Between R=20 000 and R=40 000 for metal-poor and solar-metallicity giants
Giant_MH-3_R40000_v2.pdfGiant_MH-3_R20000_v2.pdfGiant_MH0_R40000_v2.pdfGiant_MH0_R20000_v2.pdf