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SUMMARY:Neutrino Astronomy of Transient Signals
DTSTART:20170510T170000Z
DTEND:20170510T173000Z
DTSTAMP:20260412T155600Z
UID:indico-contribution-5259@events.icecube.wisc.edu
DESCRIPTION:Speakers: Anna Franckowiak (DESY)\n\nThe recent discovery of h
 igh-energy astrophysical neutrinos has opened a new window to the Universe
 . However\, the sources of those neutrinos are still unknown. Many of the 
 plausible candidates are of transient nature\, such as gamma-ray bursts\, 
 supernovae\, tidal disruption events and flares of active galactic nuclei.
  Combining neutrino data with electromagnetic (EM) measurements in a multi
 messenger approach will increase our ability to identify the neutrino sour
 ces and help to solve long-standing problems in astrophysics such as the o
 rigin of cosmic rays. The systematic search for transient signals is chall
 enging and requires regular all-sky monitoring of the EM sky or rapid real
 -time follow-up of interesting neutrino events.\nI will review the recent 
 progress in probing transient source populations as neutrino sources.\n\nh
 ttps://events.icecube.wisc.edu/event/82/contributions/5259/
LOCATION:Forum (Discovery Building)
RELATED-TO:indico-event-82@events.icecube.wisc.edu
URL:https://events.icecube.wisc.edu/event/82/contributions/5259/
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