activity
20132025
most citedAn eclipsing binary distance to the Large Magellanic Cloud accurate to 2 per cent

691 citations · 813 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2025

KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet

Cheongho Han, Andrzej Udalski, Chung-Uk Lee +29

We have investigated the lensing event KMT-2024-BLG-0404. The light curve of the event exhibited a complex structure with multiple distinct features, including two prominent causti…

astro-ph.HE2017★ 52 cited

The 2016 super-Eddington outburst of SMC X-3: X-ray and optical properties and system parameters

L. J. Townsend, J. A. Kennea, M. J. Coe +4

On 2016 July 30 (MJD 57599), observations of the Small Magellanic Cloud by Swift/XRT found an increase in X-ray counts coming from a position consistent with the Be/X-ray binary pu…

astro-ph.IM2016★ 10 cited

Analysis of photometric uncertainties in the OGLE-IV Galactic Bulge microlensing survey data

J. Skowron, A. Udalski, S. Kozłowski +8

We present a statistical assessment of both, observed and reported, photometric uncertainties in the OGLE-IV Galactic bulge microlensing survey data. This dataset is widely used fo…

astro-ph.SR2015★ 2 cited

Ultra-Short-Period Binary Systems in the OGLE Fields Toward the Galactic Bulge

I. Soszynski, K. Stepien, B. Pilecki +11

We present a sample of 242 ultra-short-period (P < 0.22 d) eclipsing and ellipsoidal binary stars identified in the OGLE fields toward the Galactic bulge. Based on the light curve…

astro-ph.CO2013★ 7 cited

Distance to the SMC from eclipsing binaries

Dariusz Graczyk, Grzegorz Pietrzynski, Bogumił Pilecki +5

The preliminary distance to a long period eclipsing binary in the Small Magellanic Cloud SMC108.1.14904 is presented. The binary system contains two non-active G-type bright giants…

astro-ph.SR2013★ 51 cited

Microlensing Discovery of a Population of Very Tight, Very Low-mass Binary Brown Dwarfs

J. -Y. Choi, C. Han, A. Udalski +121

Although many models have been proposed, the physical mechanisms responsible for the formation of low-mass brown dwarfs are poorly understood. The multiplicity properties and minim…