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20102026
most citedMOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections

235 citations · 2.5k across the 96 of their papers we have counts for

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30 papers · 1 filter

astro-ph.SR2026

A Search For Stellar-mass Black Holes Via Astrometric Microlensing II: 2012-2015 Keck Candidates

Mace J. Huston, Jessica R. Lu, Casey Y. Lam +58

The Milky Way is expected to host 10 stellar-mass black holes with an uncertain binary fraction. The only proven method to detect isolated stellar mass black holes is gra…

astro-ph.SR2026

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

Cheongho Han, Chung-Uk Lee, Andrzej Udalski +31

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 re-examination of KM…

astro-ph.SR2026

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

Cheongho Han, Andrzej Udalski, Ian A. Bond +62

We present detailed light-curve analyses of ten binary-lens microlensing events observed during the 2023--2025 seasons and selected as candidates for hosting brown-dwarf companions…

astro-ph.SR2024★ 4 cited

Millinovae: A New Class of Transient Supersoft X-ray Sources without a Classical Nova Eruption

Przemek Mróz, Krzysztof Król, Hélène Szegedi +18

Some accreting binary systems containing a white dwarf (such as classical novae or persistent supersoft sources) are seen to emit low-energy X-rays with temperatures of ~10^6 K and…

astro-ph.SR2024★ 6 cited

Observational Parameters of Blue Large-amplitude Pulsators

P. Pietrukowicz, M. Latour, I. Soszynski +15

Blue large-amplitude pulsators (BLAPs) are a recently discovered class of short-period pulsating variable stars. In this work, we present new information on these stars based on ph…

astro-ph.SR2024★ 1 cited

Discovery of the Longest-Period Classical Cepheid in the Milky Way

I. Soszyński, D. M. Skowron, A. Udalski +12

We report the discovery of the classical Cepheid OGLE-GD-CEP-1884 (= GDS_J1535467-555656) with the longest pulsation period known in our Galaxy. The period of 78.14 d is nearly 10…

astro-ph.SR2023★ 2 cited

OGLE-2017-BLG-1038: A Possible Brown-dwarf Binary Revealed by Spitzer Microlensing Parallax

Amber Malpas, Michael D. Albrow, Jennifer C. Yee +41

We report the analysis of microlensing event OGLE-2017-BLG-1038, observed by the Optical Gravitational Lensing Experiment, Korean Microlensing Telescope Network, and Spitzer telesc…

astro-ph.SR2022★ 43 cited

The OGLE Collection of Variable Stars. Nearly 66,000 Mira stars in the Milky Way

Patryk Iwanek, Igor Soszyński, Szymon Kozłowski +12

We present a collection of 65,981 Mira-type variable stars found in the Optical Gravitational Lensing Experiment (OGLE) project database. Two-thirds of our sample (40,356 objects)…

astro-ph.SR2021★ 17 cited

The OGLE Collection of Variable Stars. One Thousand Heartbeat Stars in the Galactic Bulge and Magellanic Clouds

Marcin Wrona, Milena Ratajczak, Piotr A. Kołaczek-Szymański +13

We present a collection of 991 heartbeat star (HBS) candidates found in the Optical Gravitational Lensing Experiment (OGLE) project data archive. We discuss the selection process o…

astro-ph.SR2021★ 2 cited

Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058

In-Gu Shin, Jennifer C. Yee, Kyu-Ha Hwang +30

We show that because the conditions for producing terrestrial microlens parallax (TPRX; i.e., a nearby disk lens) will also tend to produce a large lens-source relative proper moti…

astro-ph.SR2021★ 24 cited

Multiwavelength properties of Miras

Patryk Iwanek, Szymon Kozłowski, Mariusz Gromadzki +12

We comprehensively study the variability of Miras in the Large Magellanic Cloud (LMC) by simultaneous analysing light curves in 14 bands in the range of 0.524 microns. We model…

astro-ph.SR2021★ 47 cited

Binarity as the Origin of Long Secondary Periods in Red Giant Stars

I. Soszyński, A. Olechowska, M. Ratajczak +13

Long secondary periods (LSPs), observed in a third of pulsating red giant stars, are the only unexplained type of large-amplitude stellar variability known at this time. Here we sh…

astro-ph.SR2020★ 7 cited

OGLE-GAL-ACEP-091 -- The First Known Multi-Mode Anomalous Cepheid

I. Soszyński, R. Smolec, A. Udalski +12

Anomalous Cepheids (ACs) are metal-deficient, core-helium-burning pulsating stars with masses in the range 1.2-2.2 M_S. Until recently, all known ACs were pure single-mode pulsator…

astro-ph.SR2020★ 9 cited

OGLE-2018-BLG-1269Lb: A Jovian Planet With A Bright, Host

Youn Kil Jung, Andrew Gould, Andrzej Udalski +54

We report the discovery of a planet in the microlensing event OGLE-2018-BLG-1269, with planet-host mass ratio , i.e., times smaller than the Jupiter/Su…

astro-ph.SR2019★ 12 cited

Candidate Brown-dwarf Microlensing Events with Very Short Timescales and Small Angular Einstein Radii

Cheongho Han, Chung-Uk Lee, Andrzej Udalski +62

Short-timescale microlensing events are likely to be produced by substellar brown dwarfs (BDs), but it is difficult to securely identify BD lenses based on only event timescales $t…

astro-ph.SR2019★ 100 cited

Microlensing optical depth and event rate toward the Galactic bulge from 8 yr of OGLE-IV observations

P. Mroz, A. Udalski, J. Skowron +9

The number and properties of observed gravitational microlensing events depend on the distribution and kinematics of stars and other compact objects along the line of sight. In par…

astro-ph.SR2019★ 10 cited

OGLE-ing the Magellanic System: Cepheids in the Bridge

Anna M. Jacyszyn-Dobrzeniecka, I. Soszyński, A. Udalski +12

We present a detailed analysis of Magellanic Bridge Cepheid sample constructed using the OGLE Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 a…

astro-ph.SR2019★ 22 cited

OGLE-ing the Magellanic System: RR Lyrae Stars in the Bridge

Anna M. Jacyszyn-Dobrzeniecka, P. Mróz, K. Kruszyńska +12

We use the extended and updated OGLE Collection of Variable Stars to thoroughly analyze distribution of RR Lyrae stars in the Magellanic Bridge. We use photometric metallicities to…

astro-ph.SR2019★ 3 cited

OGLE-2018-BLG-0022: First Prediction of an Astrometric Microlensing Signal from a Photometric Microlensing Event

Cheongho Han, Ian A. Bond, Andrzej Udalski +63

In this work, we present the analysis of the binary microlensing event OGLE-2018-BLG-0022 that is detected toward the Galactic bulge field. The dense and continuous coverage with t…

astro-ph.SR2019★ 3 cited

OGLE-2016-BLG-0156: Microlensing Event With Pronounced Microlens-Parallax Effects Yielding Precise Lens Mass Measurement

Youn Kil Jung, Cheongho Han, Ian A. Bond +53

We analyze the gravitational binary-lensing event OGLE-2016-BLG-0156, for which the lensing light curve displays pronounced deviations induced by microlens-parallax effects. The li…

astro-ph.SR2018★ 33 cited

Microlensing Parallax for OGLE-2017-BLG-0896 Reveals a Counter-Rotating Low-Mass Brown Dwarf

Yossi Shvartzvald, Jennifer C. Yee, Jan Skowron +63

The kinematics of isolated brown dwarfs in the Galaxy, beyond the solar neighborhood, is virtually unknown. Microlensing has the potential to probe this hidden population, as it ca…

astro-ph.SR2018★ 36 cited

The OGLE Collection of Variable Stars. Classical, Type II, and Anomalous Cepheids toward the Galactic Center

I. Soszyński, A. Udalski, M. K. Szymański +11

We present a collection of classical, type II, and anomalous Cepheids detected in the OGLE fields toward the Galactic center. The sample contains 87 classical Cepheids pulsating in…

astro-ph.SR2017★ 8 cited

Concluding Henrietta Leavitt's Work on Classical Cepheids in the Magellanic System and Other Updates of the OGLE Collection of Variable Stars

I. Soszyński, A. Udalski, M. K. Szymański +9

More than a century ago, Henrietta Leavitt discovered the first Cepheids in the Magellanic Clouds together with the famous period-luminosity relationship revealed by these stars, w…

astro-ph.SR2017

Searching for Potential Mergers among 22 500 Eclipsing Binary Stars in the OGLE-III Galactic Bulge Fields

P. Pietrukowicz, I. Soszynski, A. Udalski +8

Inspired by the discovery of the red nova V1309 Sco (Nova Scorpii 2008) and the fact that its progenitor was a binary system with a rapidly decreasing orbital period, we have searc…