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Improving the Prospects for Detecting Extrasolar Planets in Gravitational Microlensing in 2002

I. A. Bond·F. Abe·R. J. Dodd·J. B. Hearnshaw·P. M. Kilmartin·K. Masuda·Y. Matsubara·Y. Muraki·S. Noda·O. K. L. Petterson·N. J. Rattenbury·M. Reid·To. Saito·Y. Saito·T. Sako·J. Skuljan·D. J. Sullivan·T. Sumi·S. Wilkinson·R. Yamada·T. Yanagisawa·P. C. M. Yock
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Abstract

Gravitational microlensing events of high magnification have been shown to be promising targets for detecting extrasolar planets. However, only a few events of high magnification have been found using conventional survey techniques. Here we demonstrate that high magnification events can be readily found in microlensing surveys using a strategy that combines high frequency sampling of target fields with online difference imaging analysis. We present 10 microlensing events with peak magnifications greater than 40 that were detected in real-time towards the Galactic Bulge during 2001 by MOA. We show that Earth mass planets can be detected in future events such as these through intensive follow-up observations around the event peaks. We report this result with urgency as a similar number of such events are expected in 2002.

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I. A. Bond, F. Abe, R. J. Dodd, J. B. Hearnshaw, P. M. Kilmartin, K. Masuda, Y. Matsubara, Y. Muraki, S. Noda, O. K. L. Petterson, N. J. Rattenbury, M. Reid, To. Saito, Y. Saito, T. Sako, J. Skuljan, D. J. Sullivan, T. Sumi, S. Wilkinson, R. Yamada, T. Yanagisawa, P. C. M. Yock. 2002-02-01. Improving the Prospects for Detecting Extrasolar Planets in Gravitational Microlensing in 2002. https://doi.org/10.1046/j.1365-8711.2002.05374.x

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