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 WAS P-4b WASP-5b OGLE-TR-113b OGLE-TR - 111b WAS P-2b WAS P-7b OGLE-TR-10 b OGLE- TR-56b 0 1 2 3 4 5 6 7 8 9 Number of observed transits 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 [email protected]
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Sergio Hoyer (1) , Patricio Rojo (1) and Mercedes López-Morales (2 ) (1): Universidad de Chile. Astronomy Department. (2): Hubble Fellow, Carnegie Institution of Washington. POSTER #86. PROYECT. OGLE-TR-111: an interesting case. - PowerPoint PPT Presentation
Transcript of Search for exoplanets using TTVs In the Southern Hemisphere
SEARCH FOR EXOPLANETS USING TTVS IN THE SOUTHERN HEMISPHERE
POSTER #86 PROYECT
WASP-4b
WASP-5b
OGLE-TR-11
3b
OGLE-TR-11
1b
WASP-2b
WASP-7b
OGLE-TR-10
b
OGLE-TR-56
b0
1
2
3
4
5
6
7
8
9
Num
ber
of o
bser
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trans
its
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
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
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
Detection of Transiting Super-Earths around Active StarsJ. Weingrill, H. Lammer, M. Khodachenko, and A. Hanslmeier
Spherical “disk” (above and below)
Forming Giant Planets by Disk Instability - Alan Boss (Carnegie Institution)
Disk with height proportional to radius (below)
