The student will take the results from an algorithmic search of the Kepler dataset and work on verifying if tagged light curves actually contain signatures from planetary transits. The light curves marked positive will then be analyzed to determine accurate size/period/eccentricity of the planet(s). Additionally, the student will use preexisting procedures to create model transits that will be injected into real light curves and then run through the search algorithm to assess our detection rate. The student will need some familiarity with IDL and coding for the second part of the project, but the first part of the project will be largely image analysis and web based providing time to pick up coding skills on the side if necessary.
Mentor: Jennifer Burt, Graduate Student
Secondary Mentor: Prof. Greg Laughlin