Results 1 to 10 of about 111 (85)

A Close Binary Lens Revealed by the Microlensing Event Gaia20bof

open access: yesThe Astronomical Journal
During the last 25 yr, hundreds of binary stars and planets have been discovered toward the Galactic bulge by microlensing surveys. Thanks to a new generation of large-sky surveys, it is now possible to regularly detect microlensing events across the ...
E. Bachelet   +27 more
doaj   +9 more sources

Twinkle: A GPU-based Binary-lens Microlensing Code with the Contour Integration Method

open access: yesThe Astrophysical Journal Supplement Series
With the rapidly increasing rate of microlensing planet detections, microlensing modeling software faces significant challenges in computation efficiency.
Suwei Wang, Lile Wang, Subo Dong
doaj   +4 more sources

OGLE-2019-BLG-0825: Constraints on the Source System and Effect on Binary-lens Parameters Arising from a Five-day Xallarap Effect in a Candidate Planetary Microlensing Event [PDF]

open access: yesThe Astronomical Journal, 2023
We present an analysis of microlensing event OGLE-2019-BLG-0825. This event was identified as a planetary candidate by preliminary modeling. We find that significant residuals from the best-fit static binary-lens model exist and a xallarap effect can fit
Yuki K. Satoh   +93 more
doaj   +7 more sources

Gaia20fnr: A binary-lens microlensing event with full orbital motion revealed by four space telescopes

open access: yesAstronomy & Astrophysics
The microlensing event Gaia20fnr is a long-duration, non-caustic-crossing binary-lens event located at a high Galactic latitude. Triggered by a photometric rise detected by the Gaia space mission, the event was followed up with observations from multiple
Wicker M.   +56 more
doaj   +3 more sources

Assessing the Impact of Binary Systems on Microlensing Using SPISEA and PopSyCLE Population Simulations

open access: yesThe Astrophysical Journal
Gravitational microlensing provides a unique opportunity to probe the mass distribution of stars, black holes, and other objects in the Milky Way. Population simulations are necessary to interpret results from microlensing surveys.
Natasha S. Abrams   +5 more
doaj   +2 more sources

A Binary Origin for the First Isolated Stellar-mass Black Hole Detected with Astrometric Microlensing

open access: yesThe Astrophysical Journal Letters, 2023
The Milky Way is believed to host hundreds of millions of quiescent stellar-mass black holes (BHs). In the last decade, some of these objects have been potentially uncovered via gravitational microlensing events.
Alejandro Vigna-Gómez   +1 more
doaj   +1 more source

Detecting Multiplanetary Systems with Gravitational Microlensing and the Roman Space Telescope

open access: yesThe Astronomical Journal, 2023
It is plausible that most of the Stars in the Milky Way Galaxy, like the Sun, consist of planetary systems, instead of a single planet. Out of the estimately discovered 3980 planet-hosting stars, about 860 of them are known to be multiplanetary systems ...
Hossein Fatheddin, Sedighe Sajadian
doaj   +1 more source

MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert

open access: yesThe Astronomical Journal, 2023
We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn mass.
Greg Olmschenk   +82 more
doaj   +1 more source

Modeling Binary Lenses and Sources with the BAGLE Python Package

open access: yesThe Astrophysical Journal
Gravitational microlensing is a powerful tool that can be used to find and measure the mass of isolated and dark compact objects. In many microlensing events, the lens, the source, or both may be binary systems.
T. Dex Bhadra   +6 more
doaj   +1 more source

Possible Gravitational Microlensing Events in the Optical Lightcurve of Active Galaxy S5 0716+714

open access: yesThe Astrophysical Journal, 2023
A well-known active galaxy of the blazar type, S5 0716+714, is characterized by a particularly high-variability duty cycle on short timescales at optical frequencies.
D. Ł. Król   +3 more
doaj   +1 more source

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