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Publikováno v: Published on 2024 May 23 by Astrophysical Journal Letters (ApJL) 967 L21

Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low insolation i

Externí odkaz: http://arxiv.org/abs/2405.14708

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