PALS: Briley Lewis, UCSB

Briley Lewis

April 6

Mon, Apr 6 2026

11:15am - 12:15pm

ATL 1250 & Zoom

 

New Tools for Debris Disk Imaging: Keck/NIRC2-Pol and GRaTer-JAX GPU Models

New Tools for Debris Disk Imaging: Keck/NIRC2-Pol and GRaTer-JAX GPU Models

Speaker: Dr. Briley Lewis, UCSB

Abstract: While protoplanetary disks reveal the earliest stages of planet formation, debris disks---like our own solar system's Kuiper Belt---provide insight into planetary evolution, such as the stage where volatiles (e.g. water) are delivered to terrestrial planets. Polarimetry is a particularly powerful technique for debris disk observations; light scattered off a dusty circumstellar disk is polarized, while the host star's light is unpolarized, creating a natural separation we can take advantage of. In this talk, I will discuss two new tools we can use for debris disk studies--the new NIRC2 polarimetry mode on the Keck II Telescope in Hawai'i that will provide cutting-edge observations of these disks, and the new GRaTer-JAX software that takes advantage of GPU computation to model debris disks-- and what we expect them to add to our understanding of planet formation and evolution.

Host: Yoni Brande


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