Showing 1–20 of 45 results
/ Date/ Name
Nov 17, 2025Sensitivity to low-mass WIMPs with an improved liquid argon ionization response model within the DarkSide programmeDec 25, 2024Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experimentJun 17, 2024The properties of AGN in dwarf galaxies identified via SED fittingJun 13, 2024Emergent Atomic Scale Polarisation Vortices in BaTiS3Apr 18, 2023The two rings of (50000) QuaoarDec 7, 2022The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementationJan 24, 2022Radio AGN in nearby dwarf galaxies: the important role of AGN in dwarf-galaxy evolutionSep 22, 2021The Forward Physics Facility: Sites, Experiments, and Physics PotentialJan 21, 2021Separating $^{39}$Ar from $^{40}$Ar by cryogenic distillation with Aria for dark matter searchesNov 19, 2018Radio-loud AGN in the first LoTSS data release: The lifetimes and environmental impact of jet-driven sourcesNov 19, 2018The origin of radio emission in broad absorption line quasars: Results from the LOFAR Two-metre Sky SurveyNov 19, 2018The LOFAR Two-metre Sky Survey - II. First data releaseNov 13, 2018The LoTSS view of radio AGN in the local Universe. The most massive galaxies are always switched onMar 11, 2018Toward Understanding the B[e] Phenomenon. VII. AS 386, a single-lined binary with a candidate black hole componentDec 6, 2017Design and Construction of the DEAP-3600 Dark Matter DetectorOct 16, 2017Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger ObservatoryOct 16, 2017A gravitational-wave standard siren measurement of the Hubble constantMay 29, 2017In-situ characterization of the Hamamatsu R5912-HQE photomultiplier tubes used in the DEAP-3600 experimentOct 4, 2016Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relationsJun 29, 2016The Herschel-ATLAS Data Release 1 Paper II: Multi-wavelength counterparts to submillimetre sources