activity
19972010
most citedDiscovery of a Jupiter/Saturn Analog with Gravitational Microlensing

366 citations · 2k across the 36 of their papers we have counts for

collaborators
Showing 2004 · astro-phShow all

11 papers · 2 filters

astro-ph2004

Microlensing Characterization of Wide-Separation Planets

Cheongho Han, B. Scott Gaudi, Jin H. An +1

With their excellent photometric precision and dramatic increase in monitoring frequency, future microlensing survey experiments are expected to be sensitive to very short time-sca…

astro-ph2004

The Microlensing Planet Finder: Completing the Census of Extrasolar Planets in the Milky Way

D. P. Bennett, I. Bond, E. Cheng +21

The Microlensing Planet Finder (MPF) is a proposed Discovery mission that will complete the first census of extrasolar planets with sensitivity to planets like those in our own sol…

astro-ph2004

On the Period Distribution of Close-In Extrasolar Giant Planets

B. Scott Gaudi, Sara Seager, Gabriela Mallen-Ornelas

Transit (TR) surveys for extrasolar planets have recently uncovered a population of ``very hot Jupiters,'' planets with orbital periods of P< 3 d. At first sight this may seem surp…

astro-ph2004

Potential Direct Single-Star Mass Measurement

H. Ghosh

We analyze the lightcurve of the microlensing event OGLE-2003-BLG-175/MOA-2003-BLG-45 and show that it has two properties that, when combined with future high resolution astrometry…

astro-ph20043 cited

Prospects for the Detection of Earth-Mass Planets

Andrew Gould, B. Scott Gaudi, Cheongho Han

We compare potential state-of-the-art experiments for detecting Earth-mass planets around main-sequence stars using radial velocities, transits, astrometry, and microlensing. For c…

astro-ph2004

OGLE-2003-BLG-238: Microlensing Mass Estimate of an Isolated Star

Guangfei Jiang, D. L. DePoy, A. Gal-Yam +38

Microlensing is the only known direct method to measure the masses of stars that lack visible companions. In terms of microlensing observables, the mass is given by M=(c^2/4G)\tild…