ANTARES upper limits on the multi-TeV neutrino emission from the GRBs detected by IACTs

Abstract

The first gamma-ray burst detections by Imaging Atmospheric Cherenkov Telescopes have been recently announced: GRB 190114C, detected by MAGIC, GRB 180720B and GRB 190829A, observed by H.E.S.S. A dedicated search for neutrinos in space and time coincidence with the gamma-ray emission observed by IACTs has been performed using ANTARES data. The search covers both the prompt and afterglow phases, yielding no neutrinos in coincidence with the three GRBs studied. Upper limits on the energetics of the neutrino emission are inferred. The resulting upper limits are several orders of magnitude above the observed gamma-ray emission, and they do not allow to constrain the available models.

accepted for publication in JCAP

References in corpus (10)

• Teraelectronvolt emission from the $\gamma$-ray burst GRB 190114C
• A very-high-energy component deep in the Gamma-ray Burst afterglow
• Observation of inverse Compton emission from a long $\gamma$-ray burst
• Time Calibration of the ANTARES Neutrino Telescope
• High-energy neutrinos from reverse shocks in choked and successful relativistic jets
• 10.4m GTC observations of the nearby VHE-detected GRB 190829A/SN 2019oyw
• Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 years of ANTARES data
• Monte Carlo simulations for the ANTARES underwater neutrino telescope
• Constraints on The Hadronic Content of Gamma Ray Bursts
• Origin of sub-TeV afterglow emission from gamma-ray bursts GRB 190114C and GRB 180720B

Cited by in corpus (4)

• Constraints on the models of the origin of high-energy astrophysical neutrinos
• Search for 10--1000 GeV neutrinos from Gamma Ray Bursts with IceCube
• GRB 221009A: Spectral signatures based on ALPs candidates
• Beyond first light: Global monitoring for high-energy neutrino astronomy