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arxiv: 1711.05298 · v1 · pith:TDNI4GGRnew · submitted 2017-11-14 · 🌌 astro-ph.IM · astro-ph.GA

Microlensing and its Degeneracy Breakers: Parallax, Finite Source, High-resolution Imaging, and Astrometry

classification 🌌 astro-ph.IM astro-ph.GA
keywords microlensingastrometrycompactdegeneracyexoplanetsarticlebasicsbeen
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First proposed by Paczynski in 1986, microlensing has been instrumental in the search of compact dark matter as well as discovery and characterization of exoplanets. In this article, we provide a brief history of microlensing, especially on the discoveries of compact objects and exoplanets. We then review the basics of microlensing and how astrometry can help break the degeneracy, providing a more robust determination of the nature of the microlensing events. We also outline prospects that will be made by on-going and forth-coming experiments/observatories

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Microlensing of fast and slow compact objects

    astro-ph.CO 2026-04 unverdicted novelty 7.0

    Microlensing surveys constrain fast and slow compact objects at masses and densities differing by orders of magnitude from dark matter limits due to speed-mass degeneracy in Einstein crossing times.