Search for neutrinos from the tidal disruption events AT2019dsg and AT2019fdr with the ANTARES telescope
arXiv:2103.15526 · doi:10.3847/1538-4357/ac16d6
Abstract
On October 1, 2019, the IceCube Collaboration detected a muon track neutrino with high probability of being of astrophysical origin, IC191001A. After a few hours, the tidal disruption event (TDE) AT2019dsg, observed by the Zwicky Transient Facility (ZTF), was indicated as the most likely counterpart of the IceCube track. More recently, the follow-up campaign of the IceCube alerts by ZTF suggested a second TDE, AT2019fdr, as a promising counterpart of another IceCube muon track candidate, IC200530A, detected on May 30, 2020. These are the second and third associations between astrophysical sources and high-energy neutrinos after the compelling identification of the blazar TXS 0506+056. Here, the search for ANTARES neutrinos from the directions of AT2019dsg and AT2019fdr using a time-integrated approach is presented. As no significant evidence for space clustering is found in the ANTARES data, upper limits on the one-flavour neutrino flux and fluence are set.
arXiv comment10 pages, 1 figure
References in corpus (21)
- The Zwicky Transient Facility: System Overview, Performance, and First Results
- Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data
- Multi-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
- Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
- Letter of Intent for KM3NeT 2.0
- The Zwicky Transient Facility: Science Objectives
- ANTARES: the first undersea neutrino telescope
- Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
- A three-dimensional calculation of atmospheric neutrinos
- A tidal disruption event coincident with a high-energy neutrino
- Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources
- First all-flavour Neutrino Point-like Source Search with the ANTARES Neutrino Telescope
- Tidally disrupted stars as a possible origin of both cosmic rays and neutrinos at the highest energies
- High-Energy Neutrino and Gamma-Ray Emission from Tidal Disruption Events
- A Family Tree of Optical Transients from Narrow-Line Seyfert 1 Galaxies
- All-flavor search for a diffuse flux of cosmic neutrinos with 9 years of ANTARES data
- A concordance scenario for the observed neutrino from a Tidal Disruption Event
- Neutrino Emission from an Off-Axis Jet Driven by the Tidal Disruption Event AT2019dsg
- Search for Neutrinos from Populations of Optical Transients
- Search for neutrinos from TXS 0506+056 with the ANTARES telescope
- Measurement of the atmospheric and energy spectra with the ANTARES neutrino telescope