Published April 2, 2021 | Version 1.0.0

Calibration of the Halpha Age-Activity relation for M dwarfs: Samples

  • 1. The Graduate Center, City University of New York
  • 2. American Museum of Natural History
  • 3. Hunter College, City University of New York
  • 4. Planétarium Rio Tinto Alcan, Espace pour la Vie
  • 5. Leibniz-Institute for Astrophysics Potsdam
  • 6. The University of North Carolina at Chapel Hill
  • 7. Macaulay Honors College, City University of New York

Description

Supplementary material to the work "Calibration of the H\(\alpha\) Age-Activity relation for M dwarfs". We include the following two samples: We compiled 89,270 M dwarfs with H\(\alpha\) equivalent widths (H\(\alpha\)EW) measurements from the literature. From this sample we were able to age-date 892 M dwarfs (1,121 including repeated stars which represent extra measurements of H\(\alpha\)EW). These ages were obtained by identifying M dwarfs which belong to known young associations, or are co-moving with a white dwarf of known age. To identify co-movers we used kinematics and parallaxes from Gaia DR2. 

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