OGLE-2016-BLG-1195 AO: Lens, Companion to Lens or Source, or None of the Above?

We systematically investigate Vandorou et al.’s claim to have detected the host star of the low-mass-ratio ( q < 10 ^−4 ) microlensing planet OGLE-2016-BLG-1195Lb, via Keck adaptive optics (AO) measurements Δ t = 4.12 yr after the event’s peak ( t _0 ). If correct, this measurement would contradict...

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Detalles Bibliográficos

Principais autores:	Andrew Gould, Yossi Shvartzvald, Jiyuan Zhang, Jennifer C. Yee, Sebastiano Calchi Novati, Weicheng Zang, Eran O. Ofek
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2023-01-01
Series:	The Astronomical Journal
Assuntos:	High-resolution microlensing event imaging Satellite microlensing parallax Gravitational microlensing exoplanet detection
Acceso en liña:	https://doi.org/10.3847/1538-3881/aced3c
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