activity
19952025
most citedMeasurement of the pressure dependence of air fluorescence emission induced by electrons

122 citations · 743 across the 23 of their papers we have counts for

collaborators

23 papers

physics.ins-det2025★ 5 cited

Spatial and Temporal Evaluations of the Liquid Argon Purity in ProtoDUNE-SP

DUNE Collaboration, S. Abbaslu, A. Abed Abud +1320

Liquid argon time projection chambers (LArTPCs) rely on highly pure argon to ensure that ionization electrons produced by charged particles reach readout arrays. ProtoDUNE Single-P…

physics.ins-det2024★ 5 cited

DUNE Phase II: Scientific Opportunities, Detector Concepts, Technological Solutions

DUNE Collaboration, A. Abed Abud, B. Abi +1366

The international collaboration designing and constructing the Deep Underground Neutrino Experiment (DUNE) at the Long-Baseline Neutrino Facility (LBNF) has developed a two-phase s…

physics.ins-det2024★ 7 cited

Doping Liquid Argon with Xenon in ProtoDUNE Single-Phase: Effects on Scintillation Light

DUNE Collaboration, A. Abed Abud, B. Abi +1317

Doping of liquid argon TPCs (LArTPCs) with a small concentration of xenon is a technique for light-shifting and facilitates the detection of the liquid argon scintillation light. I…

hep-ex2022★ 1 cited

Identification and reconstruction of low-energy electrons in the ProtoDUNE-SP detector

DUNE Collaboration, A. Abed Abud, B. Abi +1253

Measurements of electrons from interactions are crucial for the Deep Underground Neutrino Experiment (DUNE) neutrino oscillation program, as well as searches for physics beyo…

astro-ph2008★ 21 cited

A novel method for the absolute fluorescence yield measurement by AIRFLY

AIRFLY Collaboration, M. Ave

One of the goals of the AIRFLY (AIR FLuorescence Yield) experiment is to measure the absolute fluorescence yield induced by electrons in air to better than 10% precision. We introd…

astro-ph2007★ 122 cited

Measurement of the pressure dependence of air fluorescence emission induced by electrons

AIRFLY Collaboration

The fluorescence detection of ultra high energy (> 10^18 eV) cosmic rays requires a detailed knowledge of the fluorescence light emission from nitrogen molecules, which are excited…