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Cited article:

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Coronal X-Ray Emission from Nearby, Low-mass, Exoplanet Host Stars Observed by the MUSCLES and Mega-MUSCLES HST Treasury Survey Projects

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The magnetic field and multiple planets of the young dwarf AU Mic

J-F Donati, P I Cristofari, B Finociety, B Klein, C Moutou, E Gaidos, C Cadieux, E Artigau, A C M Correia, G Boué, N J Cook, A Carmona, L T Lehmann, J Bouvier, E Martioli, J Morin, P Fouqué, X Delfosse, R Doyon, G Hébrard, S H P Alencar, J Laskar, L Arnold, P Petit, Á Kóspál, et al.
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The effect of stellar contamination on low-resolution transmission spectroscopy: needs identified by NASA’s Exoplanet Exploration Program Study Analysis Group 21

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Correlating Changes in Spot Filling Factors with Stellar Rotation: The Case of LkCa 4

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Transit Timing Variations for AU Microscopii b and c

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One year of AU Mic with HARPS – II. Stellar activity and star–planet interaction

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The Mysterious Affair of the H2 in AU Mic

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One year of AU Mic with HARPS – I. Measuring the masses of the two transiting planets

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Investigating the young AU Mic system with SPIRou: large-scale stellar magnetic field and close-in planet mass

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Giant white-light flares on fully convective stars occur at high latitudes

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Magnetic Inflation and Stellar Mass. V. Intensification and Saturation of M-dwarf Absorption Lines with Rossby Number

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The UV/X-ray radiation fields and particle (CME) flows of M dwarf exoplanet host stars

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