This research has been supported by the grant PID2020-118990GB-I00 funded by MCIN/AEI/10.13039/501100011033.
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Generation of magnification maps for extragalactic microlensing studies using a fortran code based on the Poisson and Inverse Polygon method (PIP method; 2021A&A...653A.121S). The new code incorporates the presence of smoothly distributed matter, as well as two types of randomly distributed microlenses (stars and primordial black holes)
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Generation of magnification maps for extragalactic microlensing studies using a fortran code based on the Poisson and Inverse Polygon method (PIP method; 2021A&A...653A.121S). The new code incorporates the presence of smoothly distributed matter, as well as two types of randomly distributed microlenses (stars and primordial black holes)
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