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Ambiguities in fits of observed binary lens galactic microlensing events
For observed galactic microlensing events only one fit is usually presented, though, especially for a binary lens, several fits may be possible. This has been shown for the MACHO LMC#1 event (Dominik & Hirshfeld 1996). Here I discuss the strong binary lens events OGLE#7 and DUO#2.
M. Dominik
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Six binary brown dwarf candidates identified by microlensing
Astronomy & AstrophysicsIn single-lens microlensing events, the event timescale (t_ E) is typically the only measurable parameter that constrains the lens mass. Since t_ E scales with the square root of the lens mass (t_ ̊m E ∝ M^ ), a short duration may suggest a low-mass lens,
C. Han +59 more
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A Comprehensive Analysis of Three Microlensing Planet Candidates with the Planet/Binary Degeneracy
Monthly notices of the Royal Astronomical SocietyWe present observations and analyses of three high-magnification microlensing events: KMT-2022-BLG-0954, KMT-2024-BLG-0697, and MOA-2024-BLG-018. All three exhibit the “Planet/Binary” degeneracy, with planetary solutions corresponding to mass ratios in
Jiyuan Zhang +67 more
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A reference map of the human binary protein interactome
Nature, 2020Katja Luck, Dae-Kyum Kim, Luke Lambourne
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The Evolution of Compact Binary Star Systems
Living Reviews in Relativity, 2014Konstantin A Postnov
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Comparing and contrasting predictive biomarkers for immunotherapy and targeted therapy of NSCLC
Nature Reviews Clinical Oncology, 2019Ross Camidge, Robert C Doebele
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