Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
Kanata
Swift/NuSTAR
ddc:520
Astronomical Sciences
Blazar
blazar: emission
7. Clean energy
Multidisciplinary, Blazar, Neutrino
High Energy Physics - Experiment
neutrino
High Energy Physics - Experiment (hep-ex)
ASAS-SN
MISSION
High Energy Astrophysical Phenomena (astro-ph.HE)
Multidisciplinary
ORIGIN
Particle and High Energy Physics
001
Nuclear and Plasma Physics
520
Multidisciplinary Sciences
gamma ray: emission
H.E.S.S
Physical Sciences
Science & Technology - Other Topics
VERITAS
Kapteyn
Astrophysics - High Energy Astrophysical Phenomena
ACTIVE GALACTIC NUCLEI
TELESCOPE
General Science & Technology
FOS: Physical sciences
IceCube Collaboration
530
jet: relativistic
AGILE
Subaru
Neutrino
Kiso
supernova
SPECTROGRAPH
neutrino event IceCube-170922A ; gamma-ray blazar TXS 0506+056
quasar
Science & Technology
ta115
INTEGRAL
background
Institut für Physik und Astronomie
High energy neutrino
Liverpool Telescope
PERFORMANCE
VLA/17B-403 teams
MAGIC
CRAB-NEBULA
flux
messenger
gamma ray: VHE
13. Climate action
Fermi-LAT
[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
HAWC
H.E.S.S.
DOI:
10.1126/science.aat1378
Publication Date:
2018-07-12T15:05:24Z
AUTHORS (1001)
ABSTRACT
Neutrino emission from a flaring blazar
Neutrinos interact only very weakly with matter, but giant detectors have succeeded in detecting small numbers of astrophysical neutrinos. Aside from a diffuse background, only two individual sources have been identified: the Sun and a nearby supernova in 1987. A multiteam collaboration detected a high-energy neutrino event whose arrival direction was consistent with a known blazar—a type of quasar with a relativistic jet oriented directly along our line of sight. The blazar, TXS 0506+056, was found to be undergoing a gamma-ray flare, prompting an extensive multiwavelength campaign. Motivated by this discovery, the IceCube collaboration examined lower-energy neutrinos detected over the previous several years, finding an excess emission at the location of the blazar. Thus, blazars are a source of astrophysical neutrinos.
Science
, this issue p.
147
, p.
eaat1378
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