Galactic haloes in a Λ-CDM universe are predicted to host today a swarm of debris resulting
from cannibalized dwarf galaxies. The chemodynamical information recorded in their stellar …

We determined effective temperatures, surface gravities, and metallicities for a sample of
343 M dwarfs observed with CARMENES, the double-channel, high-resolution spectrograph …

Abstract The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is a
dual-hemisphere, near-infrared (NIR), spectroscopic survey with the goal of producing a …

Deriving metallicities for solar-like stars follows well-established methods, but for cooler
stars such as M dwarfs, the determination is much more complicated due to forests of …

Recent discoveries of transiting giant exoplanets around M-dwarf stars (GEMS), aided by the
all-sky coverage of TESS, are starting to stretch theories of planet formation through the core …

M dwarfs remain active over longer timescales than their Sunlike counterparts, with
potentially devastating implications for the atmospheres of their planets. However, the age at …

Exoplanets hosting M dwarfs are the best targets to characterize Earth-like or super-Earth
planetary atmospheres with the James Webb Space Telescope (JWST). We determine …

Individual chemical abundances for 14 elements (C, O, Na, Mg, Al, Si, K, Ca, Ti, V, Cr, Mn,
Fe, and Ni) are derived for a sample of M dwarfs using high-resolution, near-infrared H-band …

Detailed chemical studies of F/G/K–or solar-type–stars have long been routine in stellar
astrophysics, enabling studies in both Galactic chemodynamics and exoplanet …

Abstract The Transiting Exoplanet Survey Satellite (TESS) mission delivers time-series
photometry for millions of stars across the sky, offering a probe into stellar astrophysics …