Results 81 to 90 of about 11,007 (146)

Evolutionary algorithm-based analysis of gravitational microlensing lightcurves

open access: yes, 2012
A new algorithm developed to perform autonomous fitting of gravitational microlensing lightcurves is presented. The new algorithm is conceptually simple, versatile and robust, and parallelises trivially; it combines features of extant evolutionary ...
Asada   +56 more
core   +1 more source

Search for exoplanets in M31 with pixel-lensing and the PA-99-N2 event revisited [PDF]

open access: yes, 2010
Several exoplanets have been detected towards the Galactic bulge with the microlensing technique. We show that exoplanets in M31 may also be detected with the pixel-lensing method, if telescopes making high cadence observations of an ongoing microlensing
A. Gould   +32 more
core   +1 more source

OGLE-2014-BLG-1186: gravitational microlensing providing evidence for a planet orbiting the foreground star or for a close binary source? [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
Discussing the particularly long gravitational microlensing event OGLE-2014-BLG-1186 with a time-scale t_E ∼ 300 d, we present a methodology for identifying the nature of localised deviations from single-lens point-source light curves, which ensures that
Martin Dominik   +58 more
semanticscholar   +1 more source

The complete catalogue of light curves in equal-mass binary microlensing [PDF]

open access: yes, 2015
The light curves observed in microlensing events due to binary lenses span an extremely wide variety of forms, characterised by U-shaped caustic crossings and/or additional smoother peaks.
Bozza, Valerio   +3 more
core   +2 more sources

MACHO 96-LMC-2: Lensing of a Binary Source in the LMC and Constraints on the Lensing Object

open access: yes, 2000
We present photometry and analysis of the microlensing alert MACHO 96-LMC-2. The ~3% photometry provided by the Global Microlensing Alert Network follow--up effort reveals a periodic modulation in the lightcurve.
A. B. Tomaney   +28 more
core   +1 more source

OGLE-2017-BLG-0448Lb: A Low Mass–Ratio Wide-orbit Microlensing Planet?

open access: yesThe Astronomical Journal
The gravitational microlensing technique is most sensitive to planets in a Jupiter-like orbit and has detected more than 200 planets. However, only a few wide-orbit ( s > 2) microlensing planets have been discovered, where s is the planet-to-host ...
Ruocheng Zhai   +44 more
doaj   +1 more source

Starspot induced effects in microlensing events with rotating source star

open access: yes, 2015
We consider the effects induced by the presence of hot and cold spots on the source star in the light curves of simulated microlensing events due to either single or binary lenses taking into account the rotation of the source star and the orbital motion
De Paolis, Francesco   +3 more
core   +1 more source

The MACHO Project LMC Microlensing Results from the First Two Years and the Nature of the Galactic Dark Halo [PDF]

open access: yes, 1996
The MACHO Project is a search for dark matter in the form of massive compact halo objects (Machos). Photometric monitoring of millions of stars in the Large Magellanic Cloud (LMC), Small Magellanic Cloud (SMC), and Galactic bulge is used to search for ...
A. C. Becker   +32 more
core   +2 more sources

KMT-2016-BLG-2052L: Microlensing Binary Composed of M Dwarfs Revealed from a Very Long Timescale Event [PDF]

open access: yesAstrophysical Journal, 2018
We present the analysis of a binary microlensing event, KMT-2016-BLG-2052, for which the lensing-induced brightening of the source star lasted for two seasons.
C. Han   +28 more
semanticscholar   +1 more source

An ice giant exoplanet interpretation of the anomaly in microlensing event OGLE-2011-BLG-0173

open access: yes, 2018
We analyze the microlensing event OGLE-2011-BLG-0173, which shows a small perturbation at the end of the microlensing event caused by the primary lens. We consider both binary lens and binary source models and we explore their degeneracies, some of which
Gaudi, B. S.   +9 more
core   +1 more source

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