Recent results by the MOA group on gravitational microlensing

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dc.creatorYock, P.
dc.creatorBond, I.
dc.creatorRattenbury, N.
dc.creatorSkuljan, J.
dc.creatorSumi, T.
dc.creatorAbe, FR.
dc.creatorDodd, R.
dc.creatorHearnshaw, J.
dc.creatorHonda, M.
dc.creatorJugaku, J.
dc.creatorKilmartin, P.
dc.creatorMarles, A.
dc.creatorMasuda, K.
dc.creatorMatsubara, Y.
dc.creatorMuraki, Y.
dc.creatorNakamura, T.
dc.creatorNankivell, G.
dc.creatorNoda, S.
dc.creatorNoguchi, C.
dc.creatorOhnishi, K.
dc.creatorReid, M.
dc.creatorSaito, To.
dc.creatorSato, H.
dc.creatorSekiguchi, M.
dc.creatorSullivan, D.
dc.creatorTakeuti, M.
dc.creatorWatase, Y.
dc.creatorYanagisawa, T.
dc.date2000-07-21
dc.date2000-07-24
dc.date.accessioned2026-07-07T01:54:29Z
dc.date.available2026-07-07T01:54:29Z
dc.descriptionRecent work by the MOA gravitational microlensing group is briefly described, including (i) the current observing strategy, (ii) use of a high-speed parallel computer for analysis of results by inverse ray shooting, (iii) analysis of the light curve of event OGLE-2000-BUL12 in terms of extra-solar planets, and (iv) the MOA alert system using difference imaging.
dc.descriptionInvited paper at 9th Marcel Grossmann meeting, Rome, July 2000, 4 pages, 3 figures, uses style file ws-p9-75x6-50
dc.identifierhttps://arxiv.org/abs/astro-ph/0007317
dc.identifierhttp://arxiv.org/abs/astro-ph/0007317
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1367
dc.subjectAstrophysics
dc.titleRecent results by the MOA group on gravitational microlensing
dc.typetext

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