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19942008
most citedDiscovery of a Jupiter/Saturn Analog with Gravitational Microlensing

366 citations · 960 across the 5 of their papers we have counts for

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astro-ph2008279 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…

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-ph2008366 cited

Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing

B. S. Gaudi, D. P. Bennett, A. Udalski +66

Searches for extrasolar planets have uncovered an astonishing diversity of planetary systems, yet the frequency of solar system analogs remains unknown. The gravitational microlens…

astro-ph200520 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

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-ph2005

Asteroseismology of the Beta Cephei star Nu Eridani: photometric observations and pulsational frequency analysis

G. Handler, R. R. Shobbrook, M. Jerzykiewicz +19

We undertook a multisite photometric campaign for the Beta Cephei star Nu Eridani. More than 600 hours of differential photoelectric uvyV photometry were obtained with 11 telescope…