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asteroseismology 1galactic chemical evolution 1milky way disc 1non-lte spectroscopy 1stellar abundances 1stellar ages 1

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astro-ph.EP2025

Asteroid sizes determined with thermophysical model and stellar occultations

A. Choukroun, A. Marciniak, J. Ďurech +165

Context. The sizes of many asteroids, especially slowly rotating, low-amplitude targets, remain poorly constrained due to selection effects. These biases limit the availability of…