A neutrino with energy of $\sim$290 TeV, IceCube-170922A, was detected in coincidence with the BL Lac object TXS~0506+056 during enhanced gamma-ray activity, with chance coincidence being rejected at $\sim 3\sigma$ level. We monitored the object in the very-high-energy (VHE) band with the MAGIC telescopes for $\sim$41 hours from 1.3 to 40.4 days after the neutrino detection. Day-timescale variability is clearly resolved. We interpret the quasi-simultaneous neutrino and broadband electromagnetic observations with a novel one-zone lepto-hadronic model, based on interactions of electrons and protons co-accelerated in the jet with external photons originating from a slow-moving plasma sheath surrounding the faster jet spine. We can reproduce th...
INTRODUCTION Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and traveling at...
The IceCube event IceCube-170922A appears to originate from the BL Lac object TXS 0506+056. Despite ...
Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the ...
A neutrino with energy ∼290 TeV, IceCube-170922A, was detected in coincidence with the BL Lac object...
A neutrino with energy ∼290 TeV, IceCube-170922A, was detected in coincidence with the BL Lac object...
Abstract A neutrino with energy ~290 TeV, IceCube-170922A, was detected in coincidence with the BL ...
A neutrino with energy of ∼ 290 TeV, IceCube-170922A, was detected in coincidence with the BLLac ob...
International audienceWhile blazars have long been one of the candidates in the search for the origi...
International audienceDetection of the IceCube-170922A neutrino coincident with the flaring blazar T...
Detection of the IceCube-170922A neutrino coincident with the flaring blazar TXS 0506+056, the first...
Context. The MAGIC collaboration has recently analyzed data from a long-term multiwavelength campaig...
Individual astrophysical sources previously detected in neutrinos are limited to the Sun and the sup...
The blazar TXS 0506+056 got into the spotlight of the astrophysical community in 2017 September, whe...
Context. Many questions concerning the nature of astrophysical counterparts of high-energy neutrinos...
The blazar TXS 0506+056 got into the spotlight of the astrophysical community in 2017 September, whe...
INTRODUCTION Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and traveling at...
The IceCube event IceCube-170922A appears to originate from the BL Lac object TXS 0506+056. Despite ...
Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the ...
A neutrino with energy ∼290 TeV, IceCube-170922A, was detected in coincidence with the BL Lac object...
A neutrino with energy ∼290 TeV, IceCube-170922A, was detected in coincidence with the BL Lac object...
Abstract A neutrino with energy ~290 TeV, IceCube-170922A, was detected in coincidence with the BL ...
A neutrino with energy of ∼ 290 TeV, IceCube-170922A, was detected in coincidence with the BLLac ob...
International audienceWhile blazars have long been one of the candidates in the search for the origi...
International audienceDetection of the IceCube-170922A neutrino coincident with the flaring blazar T...
Detection of the IceCube-170922A neutrino coincident with the flaring blazar TXS 0506+056, the first...
Context. The MAGIC collaboration has recently analyzed data from a long-term multiwavelength campaig...
Individual astrophysical sources previously detected in neutrinos are limited to the Sun and the sup...
The blazar TXS 0506+056 got into the spotlight of the astrophysical community in 2017 September, whe...
Context. Many questions concerning the nature of astrophysical counterparts of high-energy neutrinos...
The blazar TXS 0506+056 got into the spotlight of the astrophysical community in 2017 September, whe...
INTRODUCTION Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and traveling at...
The IceCube event IceCube-170922A appears to originate from the BL Lac object TXS 0506+056. Despite ...
Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the ...