Search for exoplanets using TTVs In the Southern Hemisphere
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SEARCH FOR EXOPLANETS USING TTVS IN THE SOUTHERN HEMISPHERE
POSTER #86 PROYECT
WASP-4b
WASP-5b
OGLE-TR-11
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OGLE-TR-11
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WASP-2b
WASP-7b
OGLE-TR-10
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OGLE-TR-56
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OGLE-TR-111: AN INTERESTING CASE
OBSERVED – CALCULATED: CENTRAL
TIMES
Sergio Hoyer(1) , Patricio Rojo(1) and Mercedes López-Morales(2)
(1): Universidad de Chile. Astronomy Department.(2): Hubble Fellow, Carnegie Institution of Washington
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2 2Prague 08/18/2006
CARMENES – A Radial-Velocity Facility for the Calar Alto 3.5m
Three high-resolution spectrographs fed with fibers from prime focus
Search for terrestrial planets around mid-M dwarfs• Near-IR (0.95 … 1.8 μm) arm optimized for Y band• Simultaneous activity monitoring in the visible• 300 targets, 60 observations each over 5 years
Giant planets around G and K giants, up to 5 M• Multiplexed visible-light spectrograph with 14 fibers• Strong constraints for planet formation theories• 3000 targets in the M star fields
Study completed 09/15/09, awaiting review
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Post-processing of high-contrast observations of
exoplanetsSzymon Gładysz, European Southern Observatory
New algorithm for detection of faint companions in adaptive-optics observations
42m E-ELT, extreme adaptive optics, “perfect coronagraph”
long exposure after post-processing:
Poster 71
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Detection of Transiting Super-Earths around Active StarsJ. Weingrill, H. Lammer, M. Khodachenko, and A. Hanslmeier
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Spherical “disk” (above and below)
Forming Giant Planets by Disk Instability - Alan Boss (Carnegie Institution)
Disk with height proportional to radius (below)