Event Time: Monday, January 12, 2026 | 4:00 pm - 5:00 pm
Event Location:
HENN 318
Add to Calendar 2026-01-12T16:00:00 2026-01-12T17:00:00 ASTRO colloquium with Gary Bernstein Event Information: This page will be updated with the speaker's information, presentation abstract and resource links, soon! Event Location: HENN 318
Event Time: Monday, January 19, 2026 | 4:00 pm - 5:00 pm
Event Location:
HENN 318
Add to Calendar 2026-01-19T16:00:00 2026-01-19T17:00:00 ASTRO Colloquium with Samantha Lawler Event Information: This page will be updated with the speaker's information, presentation abstract and resource links, soon! Event Location: HENN 318
Event Time: Monday, February 2, 2026 | 4:00 pm - 5:00 pm
Event Location:
HENN 318
Add to Calendar 2026-02-02T16:00:00 2026-02-02T17:00:00 New Frontiers of Black Hole Feedback in Galaxy Clusters Event Information: Abstract: Galaxy clusters are fantastic laboratories for understanding black hole feedback processes. These massive cosmic structures provide a unique environment to study how AGN-driven jets transfer energy to the surrounding medium, generating shock fronts, sound waves, and turbulence. This feedback not only regulates cluster cores but also drives molecular outflows and redistributes metals within and beyond galaxies, illustrating how black holes act as the beating heart of galaxies and shape the cosmos over time. In this talk, I will review the current state of the field, focusing on how these powerful AGN-driven jets influence the properties of galaxy clusters across cosmic time. I will also present the first observations of the Perseus cluster made with the XRISM X-ray space telescope, highlighting XRISM's unprecedented capabilities in probing cluster dynamics. Lastly, I will share results from the new TNG-Cluster suite of Illustris cosmological simulations, providing new insights into the mechanisms of AGN feedback in these environments.  Bio: Dr. Julie Hlavacek-Larrondo is a leading astrophysicist at the Université de Montréal, where she heads the High-Energy and Extragalactic Astrophysics Group. She holds a prestigious Canada Research Chair in Observational Astrophysics of Black Holes, awarded to emerging world-class researchers recognized for their exceptional creativity and contributions to their fields. An expert on supermassive black holes—the titans residing at the centers of massive galaxies—Dr. Hlavacek-Larrondo combines cutting-edge machine learning techniques with observations from the world's most advanced telescopes across multiple wavelengths. Her work spans X-ray observatories like Chandra, XMM-Newton, and eROSITA; radio arrays including JVLA, GMRT, ATCA, and the upcoming SKA; and optical instruments such as Hubble Space Telescope (HST), VLT, and NASA's flagship JWST. Her research aims to unravel the complex role of black hole feedback in shaping galaxies—from regulating star formation and heating intergalactic gas to driving metal entrainment and influencing black hole growth itself. In addition, she explores a wide range of topics, including the observational signatures of radio halos in galaxy cluster mergers, the nature of hyper-luminous infrared galaxies, numerical simulations of relativistic jets, and the properties of compact objects. Before joining the Université de Montréal as a faculty member, Dr. Julie Hlavacek-Larrondo was an Einstein Fellow at Stanford University. She earned her Ph.D. from the University of Cambridge. Raised in Montreal, Julie is of Chilean and Czech heritage. Her academic journey began in 2007 with a Bachelor's degree in physics from the Université de Montréal, followed by a Master's degree in astrophysics, where she focused on the kinematical analysis of Sculptor Group galaxies. A passionate advocate for diversity in science, she recently co-founded Parité sciences, a game-changing initiative that aims to reach gender parity in sciences.    Learn More: About Julie: https://www.astro.umontreal.ca/x-tra/?team=julie-hlavacek-larrondo https://www.nserc-crsng.gc.ca/Prizes-Prix/McDonald-McDonald/Profiles-Profils/Larrondo-Larrondo_eng.asp https://www.chairs-chaires.gc.ca/chairholders-titulaires/profile-eng.aspx?profileId=3266 About Galaxy clusters: https://www.cfa.harvard.edu/research/topic/galaxy-clusters    Event Location: HENN 318
Event Time: Monday, February 9, 2026 | 4:00 pm - 5:00 pm
Event Location:
HENN 318
Add to Calendar 2026-02-09T16:00:00 2026-02-09T17:00:00 ASTRO Colloquium with Chiara Salemi Event Information: This page will be updated with the speaker's information, presentation abstract and resource links, soon! Event Location: HENN 318
Event Time: Monday, March 16, 2026 | 4:00 pm - 5:00 pm
Event Location:
HENN 318
Add to Calendar 2026-03-16T16:00:00 2026-03-16T17:00:00 A Galactic Exoplanet Census with the Roman Space Telescope Event Information:   Abstract: NASA’s Nancy Grace Roman Space Telescope, with a planned launch in late 2026, will open up unprecedented discovery space in the infrared universe. Combining Hubble-like sensitivity and resolution with a field of view 100 times larger and a sky-mapping speed 1,000 times faster, Roman will conduct panoramic, high-resolution surveys that will transform our understanding of dark energy, exoplanetary systems, galactic structure, the solar system, and star formation — all while producing an enormous data set that will be analyzed for decades to come. One of Roman’s Core Community Surveys is the Roman Galactic Bulge Time Domain Survey (RGBTDS), an ambitious program that will monitor 1.7 square degrees toward the crowded Galactic center with unprecedented precision and cadence. Over 440 days across six observing seasons, Roman will repeatedly image the same stars every 12 minutes, enabling the detection of planetary systems by using microlensing to reveal thousands of cold planets and elusive free-floating worlds, and transits to discover tens of thousands of hot and warm planets, including Earth-sized and larger worlds orbiting their stars. Together, these observations will deliver the first comprehensive galactic census of exoplanets, spanning all major stellar populations and probing planets with radii or masses above ~2× Earth’s at all separations, from hot Jupiters to icy wanderers beyond the snow line. I will highlight Roman’s revolutionary capabilities, preview its expected scientific yield, and describe the efforts of the Roman Galactic Exoplanet Survey Project Infrastructure Team (RGES-PIT), which is developing the framework, tools, and strategies to maximize the scientific return from the RGBTDS.  Bio: A member of the faculty since 2006, Prof. Gaudi is a leader in the discovery and statistical characterization of extrasolar planets using a variety of methods, including transits and gravitational microlensing. In 2008, he and his collaborators announced the discovery of the first Jupiter/Saturn analog. Prof Gaudi is deeply immersed in analytic and numerical techniques for assessing the yield, biases, and discovery potential of current and next-generation surveys to determine the demographics of exoplanets. More broadly, his interests revolve around the information content of large datasets. Prof. Gaudi is a member of the Science Definition Team for NASA’s Wide-Field Infrared Survey Telescope (WFIRST), and is the chair-elect for the NASA Exoplanet Exploration Analysis Group. Widely recognized within the community for his work, Prof. Gaudi was the 2009 recipient of the Helen B. Warner Prize of the American Astronomical Society, received NSF CAREER and PECASE awards, was named a University Distinguished Scholar in 2016, and in 2017 he was awarded the NASA Outstanding Public Leadership Medal in recognition of his "outstanding leadership as the ExoPlanet Program Analysis Group Chairperson having significant impact on NASA's search for exoplanets and life in the universe." Learn More: View his webpage from Ohio State here: https://www.astronomy.ohio-state.edu/gaudi.1/index.html About the Nancy Grace Roman Space Telescope: https://en.wikipedia.org/wiki/Nancy_Grace_Roman_Space_Telescope About the Roman Galactic Bulge Time Domain Survey (RGBTDS): https://science.nasa.gov/mission/roman-space-telescope/galactic-bulge-time-domain-survey/ About Prof. Gaudi's areas of expertise: Extrasolar planets: https://science.nasa.gov/exoplanets/ About Starlight suppression technology: https://science.nasa.gov/astrophysics/programs/exep/technology/starshade/ About Astrobiology: https://astrobiology.nasa.gov/  Event Location: HENN 318
Event Time: Monday, March 23, 2026 | 4:00 pm - 5:00 pm
Event Location:
HENN 318
Add to Calendar 2026-03-23T16:00:00 2026-03-26T17:00:00 ASTRO Colloquium with Alex Pope Event Information: This page will be updated with the speaker's information, presentation abstract and resource links, soon! Event Location: HENN 318