Slide 1Why observe M dwarfs? M9V M6V M3V M1V Due to current technical limits (~ 1m/s ---), the reflex velocities of earth-mass planets in the HZ are only observable around…
Slide 1Planet Formation Topic: Formation of gas giant planets Lecture by: C.P. Dullemond Slide 2 Two main theories Gravitational instability of the gas disk Core accretion…
Slide 1IAU Symp. 276, Torino, october 2010 R. Gratton 1, M. Kasper 2, C. Verinaud 3, M. Bonavita 1,4 + EPICS Science team Science with EPICS The E-ELT Planet Finder 1 INAF-Osservatorio…
1. intended for arxiv & ApJ on Feb 2Transit Timing Observations from Kepler : I. Statistical Analysis of the First Four MonthsarXiv:1102.0544v1 [astro-ph.EP] 2 Feb 2011…
Slide 1 Planets around Low-Mass Stars and Brown Dwarfs Michael Liu Bruce Macintosh NGAO Workshop, Sept 2006 Slide 2 2 Planets around VLM stars & brown dwarfs Direct imaging…
Comparative Performance of a 30m Groundbased GSMT and a 6.5m (and 4m) NGST NAS Committee of Astronomy & Astrophysics 9th April 2001 Matt Mountain Gemini Observatory/AURA…