BEGIN:VCALENDAR VERSION:2.0 PRODID:-//132.216.98.100//NONSGML kigkonsult.se iCalcreator 2.20.4// BEGIN:VEVENT UID:20251006T204523EDT-8978KulnAF@132.216.98.100 DTSTAMP:20251007T004523Z DESCRIPTION:Title: K-contact Distance for Noisy Nonhomogeneous Spatial Poin t Data and Application to Repeating Fast Radio Burst Sources.\n\nAbstract:  \n\nIn this talk\, I’ll introduce an approach to analyze nonhomogeneous P oisson processes (NHPP) observed with noise which focuses on previously un studied second-order characteristics of the noisy process. Utilizing a hie rarchical Bayesian model with noisy data\, we first estimate hyperparamete rs governing a physically motivated NHPP intensity. Leveraging the posteri or distribution\, we then infer the probability of detecting a certain num ber of events within a given radius\, the k-contact distance. This methodo logy is demonstrated by its motivating application: observations of fast r adio bursts (FRBs) detected by the Canadian Hydrogen Intensity Mapping Exp eriment’s FRB Project (CHIME/FRB). The approach allows us to identify repe ating FRB sources by computing the probability of observing k physically i ndependent sources within some radius in the detection domain\, or the pro bability of coincidence (PC). Applied\, the new methodology improves the r epeater detection PC\, in 86% of cases when applied to the largest sample of previously classified observations\, with a median improvement factor ( existing metric over PC from our methodology) of ~ 3000. Throughout the ta lk\, I will provide the necessary astrophysical context to motivate the ap plication and highlight some of the other active statistical problems in F RB science.\n\nSpeaker\n\nAmanda M. Cook is Banting postdoctoral fellow at the Trottier Space Institute & Physics Department at 9IÖÆ×÷³§Ãâ·Ñ an d holds a guest affiliation at the University of Amsterdam’s Anton Panneko ek Institute for Astronomy. She develops and applies statistical methodolo gy to answer questions about the nature of fast radio bursts (FRBs) and to study the otherwise invisible gas between stars and galaxies that FRBs tr avel through. \n\nhttps://mcgill.zoom.us/j/81986712072\n\nMeeting ID: 819 8671 2072\n\nPasscode: None\n\n \n DTSTART:20251010T193000Z DTEND:20251010T203000Z LOCATION:Room 1104\, Burnside Hall\, CA\, QC\, Montreal\, H3A 0B9\, 805 rue Sherbrooke Ouest SUMMARY:Amanda M. Cook (9IÖÆ×÷³§Ãâ·Ñ) URL:/sustainability/channels/event/amanda-m-cook-mcgil l-368193 END:VEVENT END:VCALENDAR