Extended Data Table 2 Properties of low metallicity LMC stars observed for short-durations on MIKE and MagE to solely derive metallicities and carbon abundances

From: Enrichment by extragalactic first stars in the Large Magellanic Cloud

  1. Derived parameters of low metallicity LMC stars observed for short durations in Extended Data Table 1. The name of the star is followed by its derived effective temperature in Kelvin (Teff), surface gravity (logg), and microturbulence in km/s (v_mic). The metallicity ([Fe/H]), carbon abundance derived from the spectrum ([C/Fe]), and carbon abundance corrected for the evolutionary state of the star ([C/Fe]_c) following ref. 31 are listed.
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