Igor Soszyński

Professor

University of Warsaw

Poland

Research Interests

Explore related searches

Professors in Poland Professors in Astronomy Astronomy professors in Poland

Contact this professor

Get a free first email built on one of their papers, ready for you to edit and send yourself.

About

Igor Soszyński is a Professor at the University of Warsaw, Poland. His research focuses on microlensing, asteroseismology, and the study of variable stars, with recent publications addressing topics such as dark matter compact objects and binary star systems. He is also involved in examining the period changes of Magellanic Cepheids and their implications for cosmological distance measurements.

Articles (20)

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2025

Year:

2024

Year:

2024

Year:

2024

Year:

2024

Year:

2023

Year:

2022

Year:

2022

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2021

Year:

2020

Collaborators (7)

Lucas Macri

Dean

The University of Texas Rio Grande Valley

UNITED STATES

View details

Jan Skowron

POLAND

View details

Chung-Uk Lee

Korea Astronomy and Space Science Institute

SOUTH KOREA

View details

Milena Ratajczak

University of Warsaw

POLAND

View details

Szymon Kozlowski

assistant professor

University of Warsaw

POLAND

View details

Lukasz Wyrzykowski

Full Professor

University of Warsaw

POLAND

View details

Mariusz Gromadzki

University of Warsaw

POLAND

View details

ApplyKite TwinLearns as you apply

Make your next move.

Prepare your application

Review drafts before you send them.

Igor Soszyński

Research Interests

Explore related searches

Contact this professor

About

Articles (20)

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

Photometric study of hot Algol-type binaries with long cycles

Observational Parameters of Blue Large-amplitude Pulsators*

Asteroseismology of Long-period Variables with OGLE-IV Data: Using Global Seismic Parameters as Luminosity Indicators

Non-evolutionary effects on period change in Magellanic Cepheids

Non-evolutionary effects on period change in Magellanic Cepheids

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

Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder

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

OGLE-ing the Magellanic System: Optical Reddening Maps of the Large and Small Magellanic Clouds from Red Clump Stars

Multiwavelength Properties of Miras

New Galactic β Lyrae-type Binaries Showing Superorbital Photometric Cycles

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

Studies of RR Lyrae Variables in Binary Systems. I. Evidence of a Trimodal Companion Mass Distribution

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

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

Collaborators (7)

Lucas Macri

Jan Skowron

Chung-Uk Lee

Milena Ratajczak

Szymon Kozlowski

Lukasz Wyrzykowski

Mariusz Gromadzki

Make your next move.