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Journal ArticleDOI

An efficient method to compute microlensed light curves for point sources

Hans J. Witt
- 01 Feb 1993 - 
- Vol. 403, Iss: 2, pp 530-541
TLDR
In this article, the authors present a method to compute microlensed light curves for point sources, where all microimages contributing to the light curve are found. But this method is not applicable to point masses in the deflector plane.
Abstract
We 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.

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Gravitational Microlensing in the Local Group

TL;DR: The status of searches for gravitational microlensing events of the stars in our galaxy and in other galaxies of the Local Group, the interpretation of the results, some theory, and prospects for the future are reviewed in this article.
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Quasar Microlensing at High Magnification and the Role of Dark Matter: Enhanced Fluctuations and Suppressed Saddle Points

TL;DR: In this paper, the authors show that diluting the stellar component of the lensing galaxy in a highly magnified system with smoothly distributed "dark" matter increases rather than decreases the microlensing fluctuations caused by the remaining stars.
Journal ArticleDOI

Gravitational Microlensing in the Local Group

TL;DR: The status of searches for gravitational microlensing events of the stars in our galaxy and in other galaxies of the Local Group, the interpretation of the results, some theory, and prospects for the future are reviewed in this article.
Journal ArticleDOI

Stokes's Theorem Applied to Microlensing of Finite Sources

TL;DR: In this paper, the computation of the magnification of a finite source by an arbitrary gravitational lens can be reduced from a two-dimensional to a one-dimensional integral using a generalization of Stokes's thereom.
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