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BEGIN:VCALENDAR VERSION:2.0 PRODID:-//Penn Engineering Events - ECPv6.18.0//NONSGML v1.0//EN CALSCALE:GREGORIAN METHOD:PUBLISH X-WR-CALNAME:Penn Engineering Events X-ORIGINAL-URL:https://seasevents.nmsdev7.com X-WR-CALDESC:Events for Penn Engineering Events REFRESH-INTERVAL;VALUE=DURATION:PT1H X-Robots-Tag:noindex X-PUBLISHED-TTL:PT1H BEGIN:VTIMEZONE TZID:America/New_York BEGIN:DAYLIGHT TZOFFSETFROM:-0500 TZOFFSETTO:-0400 TZNAME:EDT DTSTART:20180311T070000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:-0400 TZOFFSETTO:-0500 TZNAME:EST DTSTART:20181104T060000 END:STANDARD BEGIN:DAYLIGHT TZOFFSETFROM:-0500 TZOFFSETTO:-0400 TZNAME:EDT DTSTART:20190310T070000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:-0400 TZOFFSETTO:-0500 TZNAME:EST DTSTART:20191103T060000 END:STANDARD BEGIN:DAYLIGHT TZOFFSETFROM:-0500 TZOFFSETTO:-0400 TZNAME:EDT DTSTART:20200308T070000 END:DAYLIGHT BEGIN:STANDARD TZOFFSETFROM:-0400 TZOFFSETTO:-0500 TZNAME:EST DTSTART:20201101T060000 END:STANDARD END:VTIMEZONE BEGIN:VEVENT DTSTART;TZID=America/New_York:20190221T150000 DTEND;TZID=America/New_York:20190221T160000 DTSTAMP:20190212T142113Z CREATED:20190212T142113Z LAST-MODIFIED:20190212T142113Z UID:1298-1550761200-1550764800@seasevents.nmsdev7.com SUMMARY:CIS Seminar: "Cataloging the Visible Universe through Bayesian Inference at Petascale" DESCRIPTION:Abstract: \nA key task in astronomy is to locate astronomical objects in images and to characterize them according to physical parameters such as brightness\, color\, and morphology. This task\, known as cataloging\, is challenging for several reasons: many astronomical objects are much dimmer than the sky background\, labeled data is generally unavailable\, overlapping astronomical objects must be resolved collectively\, and the datasets are enormous — terabytes now\, petabytes soon. Existing approaches to cataloging are largely based on algorithmic software pipelines. In this talk\, I present a new approach to cataloging based on inference in a fully specified probabilistic model. I consider two inference procedures: one based on variational inference (VI) and another based on MCMC. A distributed implementation of VI\, written in Julia and run on a supercomputer\, achieves petascale performance — a first for any high-productivity programming language. The run is the largest-scale application of Bayesian inference reported to date. In an extension\, using new ideas from variational autoencoders and deep learning\, I avoid many of the traditional disadvantages of VI relative to MCMC\, and improve model fit URL:https://seasevents.nmsdev7.com/event/cis-seminar-cataloging-the-visible-universe-through-bayesian-inference-at-petascale/ LOCATION:Wu and Chen Auditorium (Room 101)\, Levine Hall\, 3330 Walnut Street\, Philadelphia\, PA\, 19104\, United States END:VEVENT END:VCALENDAR