Results 11 to 20 of about 107 (78)

Four-body Gravitational Microlensing Events Involving Both a Binary Lens and a Binary Source

open access: yesThe Astrophysical Journal
We present detailed analyses of three anomalous microlensing events—KMT-2021-BLG-0209, KMT-2021-BLG-0901, and OGLE-2025-BLG-0356—identified from a systematic reexamination of KMTNet light curves for which previous modeling attempts failed or left ...
Cheongho Han   +37 more
doaj   +4 more sources

First Resolution of Microlensed Images of a Binary-lens Event [PDF]

open access: yesThe Astrophysical Journal
We resolve the multiple images of the binary-lens microlensing event ASASSN-22av using the GRAVITY instrument of the Very Large Telescope Interferometer (VLTI).
Zexuan Wu   +75 more
doaj   +8 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

Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function

open access: yesThe Astronomical Journal
Gravitational microlensing is a unique method for discovering cold planets across a broad mass range. Reliable statistics of the microlensing planets require accurate sensitivity estimates.
Yuxin Shang   +7 more
doaj   +3 more sources

Candidate Microlensing Brown Dwarfs in Binary Lens Systems from the 2023–2025 Observing Seasons

open access: yesThe Astronomical Journal
We present detailed light-curve analyses of 10 binary-lens microlensing events observed during the 2023–2025 seasons and selected as candidates for hosting brown dwarf companions.
Cheongho Han   +68 more
doaj   +3 more sources

A Bayesian algorithm for model selection applied to caustic-crossing binary-lens microlensing events [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2012
We present a full Bayesian algorithm designed to perform automated searches of the parameter space of caustic-crossing binary-lens microlensing events. This builds on previous work implementing priors derived from Galactic models and geometrical considerations.
Kains, N.   +4 more
openaire   +4 more sources

Compact binaries through a lens: Silent versus detectable microlensing for the LIGO-Virgo-KAGRA gravitational wave observatories

open access: yesPhysical Review D, 2023
17 pages, 12 Figures. Updated References. Submitted to Phys.
Ruxandra Bondarescu   +3 more
openaire   +3 more sources

Dark Matter Halos from the Inside Out

open access: yesAdvances in Astronomy, Volume 2011, Issue 1, 2011., 2011
The balance of evidence indicates that individual galaxies and groups or clusters of galaxies are embedded in enormous distributions of cold, weakly interacting dark matter. These dark matter “halos” provide the scaffolding for all luminous structures in the universe, and their properties comprise an essential part of the current cosmological model.
James E. Taylor, Rob Ivison
wiley   +1 more source

Automated Detection of Short Optical Transients of Astrophysical Origin in Real Time

open access: yesAdvances in Astronomy, Volume 2010, Issue 1, 2010., 2010
The detection of short optical transients of astrophysical origin in real time is an important task for existing robotic telescopes. The faster a new optical transient is detected, the earlier follow‐up observations can be started. The sooner the object is identified, the more data can be collected before the source fades away, particularly in the most
Marcin Sokołowski   +4 more
wiley   +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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