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An efficient method to compute microlensed light curves for point sourcesWe present a method to compute microlensed light curves for point sources. This method has the general advantage that all microimages contributing to the light curve are found. While a source moves along a straight line, all micro images are located either on the primary image track or on the secondary image tracks (loops). The primary image track extends from - infinity to + infinity and is made of many sequents which are continuously connected. All the secondary image tracks (loops) begin and end on the lensing point masses. The method can be applied to any microlensing situation with point masses in the deflector plane, even for the overcritical case and surface densities close to the critical. Furthermore, we present general rules to evaluate the light curve for a straight track arbitrary placed in the caustic network of a sample of many point masses.
Document ID
19930040636
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Witt, Hans J.
(Princeton Univ. Observatory, NJ, United States)
Date Acquired
August 16, 2013
Publication Date
February 1, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 403
Issue: 2
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A24633
Funding Number(s)
CONTRACT_GRANT: NAGW-2448
CONTRACT_GRANT: NAG5-1901
CONTRACT_GRANT: DFG-AZWI-1122/1-1
Distribution Limits
Public
Copyright
Other

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