Publications (27)
Modelling the Pb release during Portland cement alteration
A. Benard, J. Rose, Jean-Louis Hazemann +6
Complex cementitious matrices undergo weathering with environmental exchange and can release metallic pollutants during alteration. The molecular mechanisms responsible for metal r…
Measurement of neutron-proton capture in the SNO+ water phase
The SNO+ Collaboration, :, M. R. Anderson +130
The SNO+ experiment collected data as a low-threshold water Cherenkov detector from September 2017 to July 2019. Measurements of the 2.2-MeV produced by neutron capture on hyd…
Discovery of Very High-Energy Gamma-Ray Radiation from the BL Lac 1ES 0806+524
VERITAS Collaboration, V. Acciari, E. Aliu +90
The high-frequency-peaked BL-Lacertae object \objectname{1ES 0806+524}, at redshift z=0.138, was observed in the very-high-energy (VHE) gamma-ray regime by VERITAS between November…
Measurement of the B Solar Neutrino Flux in SNO+ with Very Low Backgrounds
The SNO+ Collaboration, :, M. Anderson +120
A measurement of the B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with the SNO+ detector during its water commissioning phase. At energies above 6 M…
CTA Contributions to the 34th International Cosmic Ray Conference (ICRC2015)
The CTA Consortium, :, A. Abchiche +1305
List of contributions from the CTA Consortium presented at the 34th International Cosmic Ray Conference, 30 July - 6 August 2015, The Hague, The Netherlands.
Improved search for invisible modes of nucleon decay in water with the SNO+ detector
SNO+ Collaboration, :, A. Allega +116
This paper reports results from a search for single and multi-nucleon disappearance from the O nucleus in water within the \snoplus{} detector using all of the available dat…
Measurement of the B Solar Neutrino Flux Using the Full SNO+ Water Phase Dataset
SNO+ Collaboration, :, A. Allega +109
The SNO+ detector operated initially as a water Cherenkov detector. The implementation of a sealed covergas system midway through water data taking resulted in a significant reduct…
TITUS: the Tokai Intermediate Tank for the Unoscillated Spectrum
C. Andreopoulos, F. C. T. Barbato, G. Barker +75
The TITUS, Tokai Intermediate Tank for Unoscillated Spectrum, detector, is a proposed Gd-doped Water Cherenkov tank with a magnetised muon range detector downstream. It is located…
Cosmogenic Neutron Production in Water at SNO+
SNO+ Collaboration, :, M. Abreu +112
Accurate measurement of the cosmogenic muon-induced neutron yield is crucial for constraining a significant background in a wide range of low-energy physics searches. Although prev…
Evidence of Antineutrinos from Distant Reactors using Pure Water at SNO+
SNO+ Collaboration, :, A. Allega +114
The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240~km away in Ontario, Canada. This an…
First Evidence of Solar Neutrino Interactions on C
SNO+ Collaboration, :, M. Abreu +111
The SNO+ Collaboration reports the first evidence of solar neutrinos interacting on nuclei. The charged current interaction proceeds through $^{13}\t…
Event-by-Event Direction Reconstruction of Solar Neutrinos in a High Light-Yield Liquid Scintillator
A. Allega, M. R. Anderson, S. Andringa +116
The direction of individual B solar neutrinos has been reconstructed using the SNO+ liquid scintillator detector. Prompt, directional Cherenkov light was separated from the slo…
Optical calibration of the SNO+ detector in the water phase with deployed sources
SNO+ Collaboration, :, M. R. Anderson +120
SNO+ is a large-scale liquid scintillator experiment with the primary goal of searching for neutrinoless double beta decay, and is located approximately 2 km underground in SNOLAB,…
The SNO+ Experiment
SNO+ Collaboration, :, V. Albanese +251
The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta () decay will be conducted using 780 ton…
Very High Energy Gamma-Ray Emission from the Blazar Markarian 421
M. S. Schubnell, C. W. Akerlof, S. Biller J. Buckley +17
Very high energy gamma-ray emission from the BL Lac object Markarian 421 has been detected over three observing seasons on 59 nights between April 1992 and June 1994 with the Whipp…
Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)
The CTA Consortium, :, A. Abchiche +1387
List of contributions from the Cherenkov Telescope Array (CTA) Consortium presented at the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016), July 11-15,…
Current Status and Future Prospects of the SNO+ Experiment
SNO+ Collaboration, :, S. Andringa +155
SNO+ is a large liquid scintillator-based experiment located 2km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12m di…
The calibration system for the photomultiplier array of the SNO+ experiment
R. Alves, S. Andringa, S. Bradbury +20
A light injection system using LEDs and optical fibres was designed for the calibration and monitoring of the photomultiplier array of the SNO+ experiment at SNOLAB. Large volume,…
Detection of Pulsed Gamma Rays Above 100 GeV from the Crab Pulsar
VERITAS Collaboration, E. Aliu, T. Arlen +93
We report the detection of pulsed gamma rays from the Crab pulsar at energies above 100 Gigaelectronvolts (GeV) with the VERITAS array of atmospheric Cherenkov telescopes. The dete…
Initial measurement of reactor antineutrino oscillation at SNO+
SNO+ Collaboration, :, A. Allega +119
The SNO+ collaboration reports its first spectral analysis of long-baseline reactor antineutrino oscillation using 114 tonne-years of data. Fitting the neutrino oscillation probabi…
Measurement of reactor antineutrino oscillation at SNO+
SNO+ Collaboration, :, M. Abreu +298
The SNO+ collaboration reports its second spectral analysis of reactor antineutrino oscillation using 286 tonne-years of new data. The measured energies of reactor antineutrino can…
Measurement of reactor antineutrino oscillations with 1.46 ktonne-years of data at SNO+
M. Abreu, A. Allega, M. R. Anderson +108
The SNO+ Collaboration reports new results on reactor antineutrino oscillations using data acquired from May 2022 through July 2025. The spectral analysis of a flux dominated by nu…
Development, characterisation, and deployment of the SNO+ liquid scintillator
SNO+ Collaboration, :, M. R. Anderson +223
A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is…
Search for invisible modes of nucleon decay in water with the SNO+ detector
SNO+ Collaboration, :, M. Anderson +195
This paper reports results from a search for nucleon decay through 'invisible' modes, where no visible energy is directly deposited during the decay itself, during the initial wate…
Correlated variability of Mkn 421 at X-ray and TeV wavelengths on timescales of hours
L. Maraschi, G. Fossati, F. Tavecchio +26
Mkn 421 was observed for about two days with BeppoSAX, prior to and partly overlapping the start of a 1 week continuous exposure with ASCA in April 1998, as part of a world-wide mu…
A Multi-frequency campaign on the gamma-ray loud blazar W Comae
M. Maisack, K. Mannheim, R. D. Geckeler +10
We report preliminary results of a multi-frequency campaign on the TeV candidate blazar W Comae (z=0.102). Flux limits by Whipple and HEGRA show that the TeV flux must be considera…
VERITAS: Very LArge Energetic Radiation Imaging Telescope Array System
T. C. Weekes, C. Akerlof, S. Biller +37
A next generation atmospheric Cherenkov observatory is described based on the Whipple Observatory -ray telescope. A total of nine such imaging telescopes will be deployed in an…