Trinity: Probing Very High-Energy Cosmic Neutrinos with Imaging Atmospheric Cherenkov Technique

18 Jun 2024, 17:30
2h
Near Aula Magna (U6 building) (University of Milano-Bicocca)

Near Aula Magna (U6 building)

University of Milano-Bicocca

Piazza dell’Ateneo Nuovo 1, Milano, 20126
Poster Astrophysical neutrinos Poster session and reception 1

Speaker

Mariia Fedkevych (Georgia Institute of Technology)

Description

Trinity, an imaging atmospheric Cherenkov telescope (IACT) observatory, is proposed for detecting very high energy (VHE) and ultra-high energy (UHE) cosmic neutrinos.
It is designed to detect Earth-skimming tau-neutrinos, transforming into tauons which emerge in the atmosphere and decay producing air showers. Currently, Trinity is in its Demonstrator phase featuring a 0.75 m² mirror area telescope with a 5° x 5° FoV, deployed at Frisco Peak, Utah, and it promises to be the most sensitive VHE-neutrino detector for sources, pointed at NGC 1068 and TXS 0506+56. The Demonstrator became operational and started data-taking since October 3rd, 2023. This presentation highlights the Trinity Demonstrator's status, showcasing initial data acquisition results, stability, remote operation, background assessment, atmospheric monitoring, and data analysis development.

Poster prize Yes
Given name Mariia
Surname Fedkevych
First affiliation Georgia Institute of Technology
Institutional email mfedkevych3@gatech.edu
Gender Female
Collaboration (if any) Trinity

Primary author

Mariia Fedkevych (Georgia Institute of Technology)

Presentation materials