activity
20242026
collaborators

9 papers

astro-ph.EP2026

Historic microlensing events in the euclid Galactic Bulge Survey

V. Bozza, L. Salmeri, P. Rota +47

Microlensing campaigns have a long history of observations covering the Galactic bulge, where thousands of detections have been obtained, including many exoplanetary systems. The E…

astro-ph.SR2026

Thirty Circumbinary Disk Occultation Systems (KH 15D-like stars) from the OGLE Project

M. A. Urbanowicz, I. Soszyński, P. Pietrukowicz +14

We present a catalog of 30 stars that are candidates for KH 15D-like binary systems, in which the observed brightness variations are caused by a circumbinary dusty disk that period…

astro-ph.EP2026

KMT-2024-BLG-0816/OGLE-2024-BLG-0519 -- A Microlensing Event with Candidate Free-Floating Planet Lens and Blended Light

R. Poleski, Y. -H. Ryu, A. Udalski +27

We present the discovery of a free-floating planet microlensing event KMT-2024-BLG-0816. The event shows finite-source effect, significant blending light, and no microlensing signa…

astro-ph.SR2025

Doubling the Number of Blue Large-Amplitude Pulsators: Final Results of Searches for BLAPs in the OGLE Inner Galactic Bulge Fields

J. Borowicz, P. Pietrukowicz, J. Skowron +13

Blue Large-Amplitude Pulsators (BLAPs) are rare short-period (80 min) pulsating variable stars exhibiting large-amplitude brightness variations (typically between 0.1 and…

astro-ph.SR2025

Spectroscopic Observations of Four Candidates for Blue Large-Amplitude Pulsators. No BLAPs at High Galactic Latitudes

P. Pietrukowicz, M. Latour, F. Di Mille +3

We have obtained spectroscopic observations for four short-period variable objects detected in ZTF, Gaia, and Pan-STARRS (ZGP) data and classified as Blue Large-Amplitude Pulsators…

astro-ph.GA2025

Automated detection and modeling of binary microlensing events in OGLE-IV data. I. Events with well-separated bumps

R. A. P. Oliveira, R. Poleski, P. Mróz +11

Gravitational microlensing depends primarily on the lens mass and presents a larger occurrence rate in crowded regions, which makes it the best tool to uncover the initial mass fun…