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CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:1
UID:UW-Physics-Event-9740
DTSTART:20261002T203000Z
DTEND:20261002T230000Z
DTSTAMP:20261008T113731Z
LAST-MODIFIED:20260924T151737Z
LOCATION:Chamberlin 2241 - https://uwmadison.zoom.us/j/96927300636?pwd
 =2Gjt5BXqG7T3FfvBQ8C5okcNldSzzn.1
SUMMARY:Cosmology with galaxy imaging surveys: Results from the Dark E
 nergy Survey Year 6 analysis of galaxy clustering and weak lensing\, P
 hysics Department Colloquium\, Jessie Muir\, University of Cincinnati
DESCRIPTION:Over the six years of 2013-2019\, the Dark Energy Survey (
 DES) imaged one eighth of the sky\, measuring the properties of hundre
 ds of millions of galaxies. In this talk I will discuss how we leverag
 e these data to probe the geometry and growth of structure in our Univ
 erse\, and through that\, to test models describing the physics of dar
 k energy\, dark matter\, and gravity. I will present results from the 
 DES Year 6 cosmology analysis of galaxy clustering and weak gravitatio
 nal lensing\, and will highlight how\, as the largest-area galaxy imag
 ing survey of its kind\, DES serves as a laboratory for preparation fo
 r analysis with next-generation cosmological experiments like the Vera
  Rubin Observatory Legacy Survey of Space and Time (LSST). 
URL:https://www.physics.wisc.edu/events/?id=9740
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