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.
