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Deep MMT Transit Survey of the Open Cluster M37 IV: Limit on the Fraction of Stars With Planets as Small as 0.3 R_J
J. D. Hartman, B. S. Gaudi, M. J. Holman +6
We present the results of a deep (15 ~< r ~< 23), 20 night survey for transiting planets in the intermediate age open cluster M37 (NGC 2099) using the Megacam wide-field mosaic CCD…
Analytic approximations for transit light curve observables and uncertainties
Joshua A. Carter, Jennifer C. Yee, Jason Eastman +2
The light curve of an exoplanetary transit can be used to estimate the planetary radius and other parameters of interest. Because accurate parameter estimation is a non-analytic an…
Towards A Census of Earth-mass Exo-planets with Gravitational Microlensing
J. P. Beaulieu, E. Kerins, S. Mao +26
Thirteen exo-planets have been discovered using the gravitational microlensing technique (out of which 7 have been published). These planets already demonstrate that super-Earths (…
Getting More For Your Money: Identifying and Confirming Long-Period Planets with Kepler
Jennifer C. Yee, B. Scott Gaudi
Kepler will monitor enough stars that it is likely to detect single transits of planets with periods longer than the mission lifetime. We show that by combining the Kepler photomet…
A Characteristic Planetary Feature in Double-Peaked, High-Magnification Microlensing Events
Cheongho Han, B. Scott Gaudi
A significant fraction of microlensing planets have been discovered in high-magnification events, and a significant fraction of these events exhibit a double-peak structure at thei…
Characterizing Long-Period Transiting Planets Observed by Kepler
Jennifer C. Yee, B. Scott Gaudi
Kepler will monitor a sufficient number of stars that it is likely to detect single transits of planets with periods longer than the mission lifetime. We show that by combining the…