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Speagle, J · 2025 · arXiv 2503.02227

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astro-ph.SR 1

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2026 1

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UNVERDICTED 1

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Incorporating physical source parameters into microlensing modeling

astro-ph.SR · 2026-06-18 · unverdicted · novelty 6.0

A new MCMC parametrization using MIST stellar evolution models constrains source parameters in xallarap microlensing, improving Einstein ring radius estimates by up to an order of magnitude on OGLE-2017-BLG-0114 binary-source models.

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  • Incorporating physical source parameters into microlensing modeling astro-ph.SR · 2026-06-18 · unverdicted · none · ref 40

    A new MCMC parametrization using MIST stellar evolution models constrains source parameters in xallarap microlensing, improving Einstein ring radius estimates by up to an order of magnitude on OGLE-2017-BLG-0114 binary-source models.