activity
20182026
most citedCharacterization of SABRE crystal NaI-33 with direct underground counting

33 citations · 34 across the 2 of their papers we have counts for

collaborators

9 papers

hep-ex2026

Measurement of the cosmic muon flux at the Stawell Underground Physics Laboratory

G. Fu, M. Mews, F. Scutti +35

We report the first measurement of the underground cosmic muon flux at the Stawell Underground Physics Laboratory. The measurement uses eight EJ200 plastic scintillator panels, equ…

physics.ins-det2025

Photomultiplier Requirements and Pre-Calibration for the SABRE South Liquid Scintillator Veto

L. J. Milligan, P. Urquijo, E. Barberio +32

We present a study of the oil-proof base Hamamatsu R5912 photomultiplier tubes that will be used in the SABRE South linear-alkylbenzene liquid scintillator veto. SABRE South is a d…

physics.ins-det2025

Characterisation of Hamamatsu R11065-20 PMTs for use in the SABRE South NaI(Tl) Crystal Detectors

O. Stanley, W. J. D. Melbourne, P. Urquijo +31

The SABRE Experiment is a direct detection dark matter experiment using a target composed of multiple NaI(Tl) crystals. The experiment aims to be an independent check of the DAMA/L…

physics.ins-det2024

The SABRE South Technical Design Report Executive Summary

E. Barberio, T. Baroncelli, V. U. Bashu +42

In this technical design report (TDR) executive summary we describe the SABRE South detector to be built at the Stawell Underground Physics Laboratory (SUPL). The SABRE South detec…

physics.ins-det202033 cited

Characterization of SABRE crystal NaI-33 with direct underground counting

M. Antonello, I. J. Arnquist, E. Barberio +43

Ultra-pure NaI(Tl) crystals are the key element for a model-independent verification of the long standing DAMA result and a powerful means to search for the annual modulation signa…

hep-ex20201 cited

Direct search of dark matter with the SABRE experiment

Irene Bolognino

The interaction rate of hypothesised dark matter particles in an Earth-bound detector is expected to undergo an annual modulation due to the planet's orbital motion. The DAMA exper…