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20032009
most citedStudy of the decay K+ => pi+,nu,nubar in the momentum region 140<Ppi<199 MeV/c

333 citations · 532 across the 3 of their papers we have counts for

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astro-ph2008166 cited

MOA-cam3: a wide-field mosaic CCD camera for a gravitational microlensing survey in New Zealand

T. Sako, T. Sekiguchi, M. Sasaki +16

We have developed a wide-field mosaic CCD camera, MOA-cam3, mounted at the prime focus of the Microlensing Observations in Astrophysics (MOA) 1.8-m telescope. The camera consists o…

astro-ph200733 cited

Apollo asteroids (1566) Icarus and 2007 MK6: Icarus family members?

K. Ohtsuka, H. Arakida, T. Ito +6

Although it is more complicated to search for near-Earth object (NEO) families than main belt asteroid (MBA) families, since differential orbital evolution within a NEO family can…

astro-ph2005

Thermal infrared observations of the Hayabusa spacecraft target asteroid 25143 Itokawa

T. G. Mueller, T. Sekiguchi, M. Kaasalainen

We obtained N- and Q-band observations of the Apollo-type asteroid 25143 Itokawa during its close Earth approach in July 2004 with TIMMI2 at the ESO 3.6 m telescope. Our photometri…

astro-ph2005

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

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

OGLE 2003-BLG-235/MOA 2003-BLG-53: A planetary microlensing event

I. A. Bond, A. Udalski, M. Jaroszynski +29

We present observations of the unusual microlensing event OGLE 2003-BLG-235/MOA 2003-BLG-53. In this event a short duration (~7 days) low amplitude deviation in the light curve due…