activity
19972026
most citedWide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

1k citations · 5.1k across the 96 of their papers we have counts for

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Showing 2008Show all

12 papers · 1 filter

astro-ph200848 cited

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…

astro-ph20082 cited

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…

astro-ph20089 cited

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 (…

astro-ph2008

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…

astro-ph200857 cited

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…

astro-ph200843 cited

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…