Friday, July 13, 2012
12:00 pm
IPAC 102 (Large Conference Room) – David W. Morrisroe Astroscience Laboratory

IPAC Astronomy Lunch Seminar

Towards Determining eta_Earth: Characterising the Kepler Survey Completeness
Jessie Christiansen, NASA Ames
The primary goal of the Kepler mission is to determine the frequency of Earth-size planets in the habitable zones of solar-like stars. The mission has published a catalogue of planet candidates, but there are two key attributes of the catalogue that we need to understand before we can determine the underlying planet population - the rate of false negatives (completeness) and the rate of false positives (reliability). I will discuss our efforts towards determining the completeness of the survey, in particular characterising the behaviour of the automated transit detection software.
Contact Luisa Rebull at x4565
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