2011/06/28 by Y. Aita, Tsutomu Aoki, T. Aoki +23
Physics and Astronomy · #Aerospace engineering #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Cherenkov radiation #Detector #Gamma-ray bursts and supernovae #Geography #Neutrino #Neutrino Physics Research #Optics #Particle physics #Physics #Prologue #Range (aeronautics) #Satellite #astro-ph.HE
paper · pdf · doi:10.1088/2041-8205/736/1/l12
published as Astrophysical Journal Letters 736, L12 (2011) · 13 pages, 4 figures
openalex publication_date 2011/06/28 · arxiv created 2011/06/29 · arxiv updated 2011/06/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We report the first observational search for tau neutrinos (ν τ ) from gamma-ray bursts (GRBs) using one of the Ashra light collectors. The Earth-skimming ν τ technique of imaging Cherenkov τ showers was applied as a detection method. We set stringent upper limits on the ν τ fluence in PeV–EeV region for 3780 s (between 2.83 and 1.78 hr before) and another 3780 s (between 21.2 and 22.2 hr after) surrounding GRB081203A triggered by the Swift satellite. This first search for PeV–EeV ν τ complements other experiments in energy range and methodology, and suggests the prologue of "multi-particle astronomy" with a precise determination of time and location.