Near-IR and optical radial velocities of the active M-dwarf star Gl 388 (AD Leo) with SPIRou at CFHT and SOPHIE at OHP: A 2.23 day rotation period and no evidence for a co-rotating planet
and 55 more authors
É. Artigau, P. Fouqu'e, E. Martioli, C. Cadieux, J. Morin, T. Forveille, I. Boisse, G. H'ebrard, R. D'iaz, D. Lafrèniere, F. Kiefer, P. Petit, R. Doyon, L. Acuña, L. Arnold, X. Bonfils, F. Bouchy, V. Bourrier, S. Dalal, M. Deleuil, O. Demangeon, X. Dumusque, N. Hara, S. Hoyer, O. Mousis, A. Santerne, D. S'egrasan, M. Stalport, S. U. G. Alpes, France, U. Toulouse, Aix-Marseille University, Institute for Research on Exoplanets, U. Montr'eal, Canada, Observatoire du Mont-M'egantic, L. N. D. Astrof'isica, Itajub'a, Brazil, Sorbonne Universit'e, I. D. Paris, U. Montpellier, Observatoire de Geneve, Switzerland., International School for Advanced Studies, Buenos Aires, Argentina, Canada-France-Hawaii Telescope Corporation, I. D. A. E. C. D. Espacco, U. Porto, Portugal, Science Division, ESAEstec, Noordwijk, The Netherlands.
Journal: Astronomy & Astrophysics