7–11 Jul 2025
Physics Department, University of Coimbra
Europe/Lisbon timezone
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On the Detectability of Exomoons by Roman Galactic Bulge Time Domain Survey

8 Jul 2025, 11:00
15m
Auditorium C.1 (Physics Department, University of Coimbra)

Auditorium C.1

Physics Department, University of Coimbra

Rua Larga, 3004-516 Coimbra, Portugal

Speaker

Ing-Guey Jiang (National Tsing Hua University)

Description

Roman Space Telescope (formerly the Wide-Field Infrared Survey Telescope or WFIRST) is a NASA infrared space telescope scheduled to launch by May 2027. Wilson et al. (2023) predicted that Roman will find between 60000 and 200000 transiting planets. Through the simulated photometric uncertainties, the detectability of exomoons with various configurations hosted by these transiting planets will be investigated and presented.

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