Part II: ...through M dwarfs...

Telegraphic rationale. Stellar activity-planetary atmosphere interaction and effect on HZ • False-positive biosignatures (and application to upcoming targets and missions: JWST) • Radial-velocity (and photometric) follow-up: Why M dwarfs? Why NIR spectrographs? Which NIR spectrographs? HPF, SPIRou, IRD, CARMENES

Schedule (Tuesday, 14 July).

Hour Title Contributor
14:00-14:10 Welcome and introduction to satellite meeting, Part II José A. Caballero
14:10-14:25 Stellar activity of M dwarfs with planets Jorge Sanz-Forcada
(CAB, Spain)
14:25-14:40 Atmospheric chemistry of planets around M dwarfs Peter Gao
(Caltech, USA)
14:40-14:55 False positive biosignatures on habitable planets around M dwarfs Sonny Harman
(PennState, USA)
14:55-15:10 Habitable planets around M dwarfs: from Kepler to TESS, PLATO, JWST and beyond Ravi K. Kopparapu
(PennState, USA)
15:10-15:25 HPF: Habitable Planet Finder (HET) Suvrath Mahadevan
(PennState, USA)
15:25-15:40 SPIRou: SpectroPolarimétre InfraRouge (CFHT) Isabelle Boisse
(LAM/Pythéas/AMU, France)
15:40-15:55 IRD: InfraRed Doppler instrument (Subaru) Takayuki Kotani
(NAOJ, Japan)
15:55-16:10 CARMENES: Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Échelle Spectrographs (3.5m CAHA) Andreas Quirrenbach
(LSW/ZAH, Germany)
16:10-16:30 Habitable planets around M dwarfs and NIR spectrographs: synergies and future (open discussion) Convenors, contributors, all. Moderator: José A. Caballero

Contact for Part II.