Microlensing optical depth and event rate toward the Large Magellanic Cloud based on 20 years of OGL...
Microlensing optical depth and event rate toward the Large Magellanic Cloud based on 20 years of OGLE observations
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Author / Creator
Mroz, P , Udalski, A , Szymanski, M K , Kapusta, M , Soszynski, I , Wyrzykowski, L , Pietrukowicz, P , Kozlowski, S , Poleski, R , Skowron, J , Skowron, D , Ulaczyk, K , Gromadzki, M , Rybicki, K , Iwanek, P , Wrona, M and Ratajczak, M
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
Measurements of the microlensing optical depth and event rate toward the Large Magellanic Cloud (LMC) can be used to probe the distribution and mass function of compact objects in the direction toward that galaxy - in the Milky Way disk, the Milky Way dark matter halo, and the LMC itself. The previous measurements, based on small statistical sample...
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Full title
Microlensing optical depth and event rate toward the Large Magellanic Cloud based on 20 years of OGLE observations
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Record Identifier
TN_cdi_proquest_journals_2938146180
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2938146180
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.2403.02398
