Szymon Kozlowski

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assistant professor

University of Warsaw

Poland

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About

Dr. Szymon Kozlowski is an assistant professor at Warsaw University, Poland. His research focuses on astrophysics, specifically in microlensing, black hole characteristics, and stellar movements in the Milky Way and Magellanic Clouds. Recent publications highlight topics such as transient supersoft X-ray sources and the optical depth related to compact objects in dark matter.

Recent Grants

Grant: Close

Aperiodic Variability in OGLE, Gaia and LSST

Open Date: 2019-08-01

Close Date: 2022-07-01

Grant: Close

Extragalactic Astrophysics with OGLE

Open Date: 2015-07-01

Close Date: 2019-07-01

Articles (16)

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2025

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2024

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2024

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2024

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2024

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2024

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2024

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2023

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2022

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2022

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2022

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2022

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2022

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2021

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2021

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2020

Collaborators (8)

Jan Skowron

POLAND

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Tobias C. Hinse

University of Southern Denmark

DENMARK

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Chung-Uk Lee

Korea Astronomy and Space Science Institute

SOUTH KOREA

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Milena Ratajczak

University of Warsaw

POLAND

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Lukasz Wyrzykowski

Full Professor

University of Warsaw

POLAND

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Mariusz Gromadzki

University of Warsaw

POLAND

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Eamonn Kerins

The University of Manchester

UNITED KINGDOM

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Igor Soszyński

Professor

University of Warsaw

POLAND

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Szymon Kozlowski

Research Interests

Explore related searches

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About

Recent Grants

Articles (16)

Microlensing Optical Depth, Event Rate, and Limits on Compact Objects in Dark Matter Based on 20 Yr of OGLE Observations of the Small Magellanic Cloud

No massive black holes in the Milky Way halo

Microlensing Optical Depth and Event Rate toward the Large Magellanic Cloud Based on 20 yr of OGLE Observations

Limits on Planetary-mass Primordial Black Holes from the OGLE High-cadence Survey of the Magellanic Clouds

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

Virial Black Hole Masses for Active Galactic Nuclei behind the Magellanic Clouds

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

A Three-dimensional Map of the Milky Way Using 66,000 Mira Variable Stars

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

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

Photometric Analysis of the OGLE Heartbeat Stars

An Isolated Mass-gap Black Hole or Neutron Star Detected with Astrometric Microlensing

An Isolated Stellar-mass Black Hole Detected through Astrometric Microlensing

Multiwavelength Properties of Miras

Mid-infrared Period–Luminosity Relations for Miras in the Large Magellanic Cloud

A Terrestrial-mass Rogue Planet Candidate Detected in the Shortest-timescale Microlensing Event

Collaborators (8)

Jan Skowron

Tobias C. Hinse

Chung-Uk Lee

Milena Ratajczak

Lukasz Wyrzykowski

Mariusz Gromadzki

Eamonn Kerins

Igor Soszyński

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