BEGIN:VCALENDAR VERSION:2.0 PRODID:-//wp-events-plugin.com//7.4.5//EN TZID:America/Los_Angeles X-WR-TIMEZONE:America/Los_Angeles BEGIN:VEVENT UID:0-1879@hmc.edu DTSTART;TZID=America/Los_Angeles:20261204T110000 DTEND;TZID=America/Los_Angeles:20261204T120000 DTSTAMP:20261113T231510Z URL:https://www.hmc.edu/calendar/events/cs-colloquium-images-of-the-hidden -universe-katie-bouman-caltech/ SUMMARY:CS Colloquium: “Images of the Hidden Universe\,” Katie Bouman\, Caltech DESCRIPTION:At the heart of our Milky Way galaxy lies a supermassive black hole called Sagittarius A* that is evolving on the timescale of mere minut es. Computer scientist Katie Bouman will present the methods and procedure s used to produce the first images of Sagittarius A* as well as discuss fu ture directions we are taking to leverage machine learning to sharpen our view of the black hole\, including mapping its evolving environment in 3D. \n\nIt has been theorized for decades that a black hole will leave a "shad ow" on a background of hot gas. However\, due to its small size\, traditio nal imaging approaches require an Earth-sized radio telescope. In this tal k\, Bouman discusses techniques developed to photograph a black hole using the Event Horizon Telescope\, a network of telescopes scattered across th e globe. Recovering an image from this data requires solving an ill-posed inverse problem which necessitates the use of image priors to reduce the s pace of possible solutions. Although we have learned a lot from these init ial images already\, remaining scientific questions motivate us to improve this computational telescope to see black hole phenomena still invisible to us. She will discuss approaches developed to incorporate data-driven di ffusion model priors into the imaging process to sharpen the view of the b lack hole and understand the sensitivity of the image to different underly ing assumptions. Additionally\, she will discuss how her team has develope d techniques that allow them to extract the evolving structure of our own Milky Way’s black hole over the course of a night. She will introduce Or bital Black Hole Tomography\, which integrates known physics with a neural representation to map evolving flaring emission around the black hole in 3D for the first time.\nSpeaker\nKatherine L. (Katie) Bouman is a professo r in the Computing and Mathematical Sciences\, Electrical Engineering and Astronomy departments at the California Institute of Technology. Her work combines ideas from signal processing\, computer vision\, machine learning and physics to find and exploit hidden signals for scientific discovery. Before joining Caltech\, she was a postdoctoral fellow in the Harvard-Smit hsonian Center for Astrophysics. She received her PhD in the Computer Scie nce and Artificial Intelligence Laboratory (CSAIL) at MIT in EECS\, and he r bachelor's degree in electrical engineering from the University of Michi gan. She is a Rosenberg Scholar\, Heritage Medical Research Institute Inve stigator\, recipient of the Royal Photographic Society Progress Medal\, El ectronic Imaging Scientist of the Year Award\, Sloan Fellowship\, Universi ty of Michigan Outstanding Recent Alumni Award and co-recipient of the Bre akthrough Prize in Fundamental Physics. As part of the Event Horizon Teles cope Collaboration\, she co-led the Imaging Working Group and acted as coo rdinator for papers concerning the first imaging of the M87* and Sagittari us A* black holes. CATEGORIES:Faculty,Staff,Students LOCATION:Galileo Hall\, 240 Platt Blvd.\, Claremont\, CA\, 91711\, United S tates X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=240 Platt Blvd.\, Claremont \, CA\, 91711\, United States;X-APPLE-RADIUS=100;X-TITLE=Galileo Hall:geo: 0,0 END:VEVENT BEGIN:VTIMEZONE TZID:America/Los_Angeles X-LIC-LOCATION:America/Los_Angeles BEGIN:STANDARD DTSTART:20261101T010000 TZOFFSETFROM:-0700 TZOFFSETTO:-0800 TZNAME:PST END:STANDARD END:VTIMEZONE END:VCALENDAR