activity
20032012
most citedOGLE 2003-BLG-235/MOA 2003-BLG-53: A planetary microlensing event

396 citations · 710 across the 9 of their papers we have counts for

collaborators

9 papers

hep-ph2012★ 13 cited

Averaged Number of the Lightest Supersymmetric Particles in Decay of Superheavy Particle with Long Lifetime

Yasuhiro Kurata, Nobuhiro Maekawa

We calculate the averaged number νof the lightest supersymmetric particles (LSPs) in a shower from the decay of superheavy particle X by generalized DGLAP equations. If the primary…

astro-ph2005★ 65 cited

GRB 021004 modelled by multiple energy injections

A. de Ugarte Postigo, A. J. Castro-Tirado, J. Gorosabel +43

GRB 021004 is one of the best sampled gamma-ray bursts (GRB) to date, although the nature of its light curve is still being debated. Here we present a large amount (107) of new opt…

astro-ph2005★ 20 cited

Determination of stellar shape in microlensing event MOA 2002-BLG-33

N. J. Rattenbury, F. Abe, D. P. Bennett +30

We report a measurement of the shape of the source star in microlensing event MOA 2002-BLG-33. The lens for this event was a close binary whose centre-of-mass passed almost directl…

astro-ph2005★ 11 cited

Multiple Outbursts of a Cataclysmic Variable in the Globular Cluster M22

I. A. Bond, F. Abe, S. Eguchi +18

We present a 4 year light curve of a cataclysmic variable in M22, based on an analysis of accumulated data from the MOA microlensing survey. The position of the star coincides with…

astro-ph2004★ 50 cited

Search for Low-Mass Exoplanets by Gravitational Microlensing at High Magnification

F. Abe, D. P. Bennett, I. A. Bond +32

Observations of the gravitational microlensing event MOA 2003-BLG-32/OGLE 2003-BLG-219 are presented for which the peak magnification was over 500, the highest yet reported. Contin…

astro-ph2004★ 42 cited

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…