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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-9637
DTSTART:20260430T193000Z
DTEND:20260430T210000Z
DTSTAMP:20260413T083721Z
LAST-MODIFIED:20260330T202457Z
LOCATION:5280 CH
SUMMARY:Measurement of the Neutrino Flux from the Milky Way using the 
 IceCube Multi-Flavor Astrophysical Neutrino Sample\, Preliminary Exam\
 , Matthias Thiesmeyer\, Physics PhD Graduate Student
DESCRIPTION:The IceCube Neutrino Observatory has provided new insights
  into the high-energy universe\, unveiling neutrinos from the galactic
  plane to extragalactic supermassive black holes. In this talk\, we pr
 esent a 12.3-year\, full-sky\, all-flavor dataset\, the IceCube Multi-
 Flavor Astrophysics Neutrino sample (ICEMAN). ICEMAN is the combinatio
 n of three largely independent neutrino samples of different event mor
 phologies. It builds upon the previous work of the DNN-based cascade s
 ample\, Enhanced Starting Track Event Selection\, and the Northern Tra
 ck sample. Recent improvements in ice modeling and detector calibratio
 n are also incorporated into the cascade simulation and reconstruction
 . This dataset was used in an unbinned maximum likelihood to carry out
  a template-based measurement of the diffuse galactic neutrino flux ac
 ross four distinct model hypotheses. Preliminary measurement results w
 ill be presented\, addressing the different model assumptions.    Furt
 hermore\, prospects of a follow-up analysis targeting the galactic cen
 ter using enhancements in background simulation will be discussed.
URL:https://www.physics.wisc.edu/events/?id=9637
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