scispace - formally typeset
P

P. Browne

Researcher at University of St Andrews

Publications -  48
Citations -  2125

P. Browne is an academic researcher from University of St Andrews. The author has contributed to research in topics: Gravitational microlensing & Light curve. The author has an hindex of 25, co-authored 48 publications receiving 2023 citations. Previous affiliations of P. Browne include Las Cumbres Observatory Global Telescope Network.

Papers
More filters
Journal ArticleDOI

MOA-2009-BLG-387Lb: a massive planet orbiting an M dwarf

V. Batista, +148 more
TL;DR: In this article, the authors reported the discovery of a planet with a high planet-to-star mass ratio in the microlensing event MOA-2009-BLG-387, which exhibited pronounced deviations over a 12-day interval.
Journal ArticleDOI

Binary Microlensing Event OGLE-2009-BLG-020 Gives Verifiable Mass, Distance, and Orbit Predictions

Jan Skowron, +108 more
TL;DR: In this article, the first example of binary microlensing for which the parameter measurements can be verified (or contradicted) by future Doppler observations is presented, made possible by a confluence of two relatively unusual circumstances.
Journal ArticleDOI

MOA-2011-BLG-262Lb: A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge

David P. Bennett, +101 more
TL;DR: In this paper, the first microlensing candidate for a free-floating exoplanet-exomoon system, MOA-2011-BLG-262, with a primary lens mass of M host ~ 4 Jupiter masses hosting a sub-Earth mass moon was presented.
Journal ArticleDOI

Discovery and mass measurements of a cold, 10 earth mass planet and its host star

Yasushi Muraki, +129 more
TL;DR: In this article, the discovery and mass measurement of the cold, low-mass planet MOA-2009-BLG-266Lb, made with the gravitational microlensing method, is presented.
Journal ArticleDOI

Binary microlensing event OGLE-2009-BLG-020 gives a verifiable mass, distance and orbit predictions

TL;DR: In this article, the first example of binary microlensing for which the parameter measurements can be verified (or contradicted) by future Doppler observations is presented, made possible by a confluence of two relatively unusual circumstances.