Pa Chia Thao

TL;DR: The mass-luminosity relation for late-type stars has long been a critical tool for estimating stellar masses as mentioned in this paper, and there is a growing need for both a higher-precision relation and a better understanding of systematic effects (e.g., metallicity).

TL;DR: In this article, the authors presented the discovery of a transiting planet larger than Neptune but smaller than Saturn in the 45 Myr Tucana-Horologium young moving group, where the host star is a visual binary, and follow-up observations demonstrate that the planet orbits the G6V primary component, DS Tuc A (HD 222259A, TIC 410214986).

TL;DR: In this paper, the authors presented the discovery of a transiting planet larger than Neptune but smaller than Saturn in the 45 Myr Tucana-Horologium young moving group, where the host star is a visual binary and follow-up observations demonstrate that the planet orbits the G6V primary component, DS Tuc A (HD 222259A, TIC 410214986).

TL;DR: In this paper, the authors used the National Science Foundation Graduate Research Fellowship Program (GRF) under grant No. DGE-1650116 to support the work of P.A.W.V.