Search results for "multi-messenger astronomy"

showing 2 items of 2 documents

SNEWS 2.0 : a next-generation supernova early warning system for multi-messenger astronomy

2021

The next core-collapse supernova in the Milky Way or its satellites will represent a once-in-a-generation opportunity to obtain detailed information about the explosion of a star and provide significant scientific insight for a variety of fields because of the extreme conditions found within. Supernovae in our galaxy are not only rare on a human timescale but also happen at unscheduled times, so it is crucial to be ready and use all available instruments to capture all possible information from the event. The first indication of a potential stellar explosion will be the arrival of a bright burst of neutrinos. Its observation by multiple detectors worldwide can provide an early warning for t…

Milky WayAstrophysics::High Energy Astrophysical PhenomenasatelliteFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - Experiment010305 fluids & plasmasHigh Energy Physics - Experiment (hep-ex)Astronomi astrofysik och kosmologistar0103 physical sciencessupernova[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astronomy Astrophysics and Cosmology010306 general physicssupernova neutrinoscaptureAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsWarning systemSupernova Early Warning SystembackgroundAstronomysensitivityGalaxySupernovaelectromagneticNeutrino detectorsupernova neutrinos; multi-messenger astronomy; particle astrophysicsneutrino: burstgalaxyNeutrinoAstrophysics - High Energy Astrophysical Phenomenamulti-messenger astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]particle astrophysics
researchProduct

The IceCube realtime alert system

2016

Following the detection of high-energy astrophysical neutrinos in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the IceCube neutrino observatory. Several analyses selecting neutrinos of astrophysical origin are now operating in realtime at the detector site in Antarctica and are producing alerts to the community to enable rapid follow-up observations. The goal of these observations is to locate the astrophysical objects responsible for these neutrino signals. This paper highlights the infrastructure in place both at the South Pole detector site and at IceC…

HIGH-ENERGY NEUTRINOSTELESCOPEAstrophysics::High Energy Astrophysical PhenomenaMulti-messenger astronomy; Neutrino astronomy; Neutrino detectors; Transient sources; Astronomy and AstrophysicspoleFOS: Physical sciences01 natural sciencesIceCubelaw.inventionIceCube Neutrino ObservatoryTelescopeSEARCHESCORE-COLLAPSE SUPERNOVAElawObservatory0103 physical sciencesMulti-messenger astronomysiteNeutrino detectors010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsbackgroundEvent (computing)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsPERFORMANCEsensitivityTransient sourcesobservatoryIdentification (information)electromagneticPhysics and AstronomyNeutrino detectorNeutrino astronomyddc:540High Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsFOLLOW-UPAstroparticle Physics
researchProduct