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Integrated Mass Loss for Very Metal-poor Stars: Asterosesimic Red Giant Masses of K2 Globular Cluster NGC 5897

  • Authors: Csilla Kalup, László Molnár, Madeline Howell, Attila Bódi, András Pál

Csilla Kalup et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure D1.

We resampled the original mass distribution of RGB stars (light pink curve) to create new mass distributions of N = 4 small-sized subsamples (purple curves). The dashed lines represent the peaks of each distribution. After 100,000 random realizations, the purple peak values were used to characterize the uncertainty in the average EAGB mass introduced by small number statistics. This is an example of 16 random realizations. See Appendix D for more details.

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