The Inverse Problem in Microlensing

Details The Inverse Problem in Microlensing The Inverse Problem in Microlensing

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet.2133c&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

We present a simple method to obtain informations on galaxy models parameters using the measured value of the microlensing optical depth and the number of observed events and taking also into account problems connected with the detection efficiency: inverse problem in microlensing. We apply this technique to the class of power - law models with nearly flat rotation curve to reduce the whole parameter space (q, Rc) compatible with the measures of τobsd and Nevobsd towards LMC.

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