activity
19972016
most citedOGLE 2003-BLG-235/MOA 2003-BLG-53: A planetary microlensing event

396 citations · 1.8k across the 36 of their papers we have counts for

collaborators

36 papers

astro-ph.EP2016★ 9 cited

OGLE-2012-BLG-0724Lb: A Saturn-mass Planet around an M-dwarf

Y. Hirao, A. Udalski, T. Sumi +35

We report the discovery of a planet by the microlensing method, OGLE-2012-BLG-0724Lb. Although the duration of the planetary signal for this event was one of the shortest seen for…

astro-ph.EP2016★ 25 cited

Spitzer Observations of OGLE-2015-BLG-1212 Reveal a New Path to Breaking Strong Microlens Degeneracies

V. Bozza, Y. Shvartzvald, A. Udalski +98

Spitzer microlensing parallax observations of OGLE-2015-BLG-1212 decisively breaks a degeneracy between planetary and binary solutions that is somewhat ambiguous when only ground-b…

astro-ph.EP2015★ 5 cited

Reanalyses of Anomalous Gravitational Microlensing Events in the OGLE-III Early Warning System Database with Combined Data

J. Jeong, H. Park, C. Han +95

We reanalyze microlensing events in the published list of anomalous events that were observed from the OGLE lensing survey conducted during 2004-2008 period. In order to check the…

astro-ph.SR2009★ 1 cited

Energy Determination of Solar Neutrons by the SEDA-AP on-board JEM of ISS

K. Koga, T. Goka, H. Matsumoto +3

A solar neutron detector has been launched on the Japan Exposure Module (JEM) of the International Space Station (ISS) in August 4, 2009. The detector works satsifactory. The detec…

astro-ph.HE2009

Contribution of Stellar Flares to the Diffuse Component of Galactic Gamma-Rays

Y. Muraki

It is well known that the diffuse gamma-rays are produced by the collisions between the galactic cosmic rays with the stellar matter (Hayakawa-Morrison Hypothesis). In this paper t…

astro-ph2008★ 279 cited

A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192

D. P. Bennett, I. A. Bond, A. Udalski +44

We report the detection of an extrasolar planet of mass ratio q ~ 2 x 10^(-4) in microlensing event MOA-2007-BLG-192. The best fit microlensing model shows both the microlensing pa…