Exoplanet Occurrence Rates from Microlensing Surveys

Fuente: arXiv
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Auteurs principaux: Mroz, P., Poleski, R.
Format: Preprint
Publié: 2023
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author Mroz, P.
Poleski, R.
author_facet Mroz, P.
Poleski, R.
contents The number of exoplanets detected using gravitational microlensing technique is currently larger than 200, which enables population studies. Microlensing is uniquely sensitive to low-mass planets orbiting at separations of several astronomical units, a parameter space that is not accessible to other planet-detection techniques, as well as free-floating planets, not orbiting around any star. In this review, we present the state-of-the-art knowledge on the demographics of exoplanets detected with microlensing, with a particular emphasis on their occurrence rates. We also summarize the current knowledge about free-floating planets, an elusive population of objects that seem to be more common than ordinary, gravitationally bound exoplanets.
format Preprint
id arxiv_https___arxiv_org_abs_2310_07502
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Exoplanet Occurrence Rates from Microlensing Surveys
Mroz, P.
Poleski, R.
Earth and Planetary Astrophysics
Astrophysics of Galaxies
The number of exoplanets detected using gravitational microlensing technique is currently larger than 200, which enables population studies. Microlensing is uniquely sensitive to low-mass planets orbiting at separations of several astronomical units, a parameter space that is not accessible to other planet-detection techniques, as well as free-floating planets, not orbiting around any star. In this review, we present the state-of-the-art knowledge on the demographics of exoplanets detected with microlensing, with a particular emphasis on their occurrence rates. We also summarize the current knowledge about free-floating planets, an elusive population of objects that seem to be more common than ordinary, gravitationally bound exoplanets.
title Exoplanet Occurrence Rates from Microlensing Surveys
topic Earth and Planetary Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2310.07502