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Stellar, remnant, planetary, and dark-object masses from astrometric microlensing

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dc.contributor.author Boden, A. en_US
dc.contributor.author Gould, A. P. en_US
dc.contributor.author Bennett, D. P. en_US
dc.contributor.author Depoy, D. L. en_US
dc.contributor.author Gaudi, S. B. en_US
dc.contributor.author Griest, K. en_US
dc.contributor.author Han, C. en_US
dc.contributor.author Paczynski, B. en_US
dc.contributor.author Reid, I. N. en_US
dc.date.accessioned 2004-09-17
dc.date.available 2004-09-17
dc.date.issued 2002-01-06 en_US
dc.identifier.citation 199th American Astronomical Society Meeting en_US
dc.identifier.citation Washington D.C., USA en_US
dc.identifier.clearanceno 02-0011 en_US
dc.identifier.uri http://hdl.handle.net/2014/8070
dc.description.abstract With SIM, we will break the microlensing degeneracy, and allow detailed interpretation of individual microlensing events. We will thus develop a detailed census of the dark and luminous stellar population of the Galaxy. en_US
dc.format.extent 2434490 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Space Interferometry Mission science en_US
dc.title Stellar, remnant, planetary, and dark-object masses from astrometric microlensing en_US


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