| First results from the NEWS-G direct dark matter search experiment at the LSM |
21 |
| Design and construction of the DEAP-3600 dark matter detector |
15 |
| Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources |
10 |
| Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout |
10 |
| Revealing neutral bremsstrahlung in two-phase argon electroluminescence |
9 |
| On the claim of modulations in radon decay and their association with solar rotation |
9 |
| Constraints on the cosmic distance duality relation with simulated data of gravitational waves from the Einstein Telescope |
9 |
| The on-orbit calibration of DArk Matter Particle Explorer |
8 |
| A deep learning-based reconstruction of cosmic ray-induced air showers |
8 |
| The Monte Carlo simulation of the Borexino detector |
7 |
| On-orbit operations and offline data processing of CALET onboard the ISS |
6 |
| Response of photomultiplier tubes to xenon scintillation light |
6 |
| Charge measurement of cosmic ray nuclei with the plastic scintillator detector of DAMPE |
6 |
| Slow liquid scintillator candidates for MeV-scale neutrino experiments |
6 |
| Monte Carlo simulation of the SABRE PoP background |
6 |
| Study and mitigation of spurious electron emission from cathodic wires in noble liquid time projection chambers |
6 |
| Search for WIMP-Xe-129 inelastic scattering with particle identification in XMASS-I |
6 |
| Constraints on the diffuse photon flux with energies above 10(18) eV using the surface detector of the Telescope Array experiment |
6 |
| Cosmogenic production of tritium in dark matter detectors |
5 |
| The muon intensity in the Felsenkeller shallow underground laboratory |
5 |
| Extended Lambda CDM model |
5 |
| Analysis of gamma radiation from a radon source. II: Indications of influences of both solar and cosmic neutrinos on beta decays |
5 |
| Investigation of very high energy cosmic rays by means of inclined muon bundles |
4 |
| Production rate measurement of Tritium and other cosmogenic isotopes in Germanium with CDMSlite |
4 |
| Limits on the flux of tau neutrinos from 1 PeV to 3 EeV with the MAGIC telescopes |
4 |
| Application of deep learning methods to analysis of imaging atmospheric Cherenkov telescopes data |
4 |
| Present and projected sensitivities of Dark Matter direct detection experiments to effective WIMP-nucleus couplings |
4 |
| Quenching factor measurement for NaI(Tl) scintillation crystal |
4 |
| Chromatographic separation of radioactive noble gases from xenon |
4 |
| In-flight energy calibration of the space-borne Compton polarimeter POLAR |
4 |
| Low-background gamma spectroscopy at the Boulby Underground Laboratory |
4 |
| Spectral features in the cosmic ray fluxes |
4 |
| Deep learning techniques applied to the physics of extensive air showers |
3 |
| Calibration of the LOFAR low-band antennas using the Galaxy and a model of the signal chain |
3 |
| Performance measurement of HARPO: A time projection chamber as a gamma-ray telescope and polarimeter |
3 |
| Nature of the low-energy, gamma-like background for the Cherenkov Telescope Array |
3 |
| Phase-matching of multiple-cavity detectors for dark matter axion search |
3 |
| Probing a steep EoS for dark energy with latest observations |
3 |
| Study of short term enhanced TeV gamma- ray emission from Mrk 421 observed with TACTIC on December 2014 |
3 |
| On the origin of particle fluxes from thunderclouds |
3 |
| Sensitivity of the PICO-500 bubble chamber to supernova neutrinos through coherent nuclear elastic scattering |
3 |
| Sensitivity of carbon and oxygen yields to the triple-alpha resonance in massive stars |
3 |
| Measuring the Galactic Cosmic Ray flux with the LISA Pathfinder radiation monitor |
3 |
| Production and propagation of ultra-high energy photons using CRPropa 3 |
3 |
| On the potential of Cherenkov Telescope Arrays and KM3 Neutrino Telescopes for the detection of extended sources |
3 |
| Naturally occurring Si-32 and low-background silicon dark matter detectors |
2 |
| Background studies of high energy gamma rays from (n,gamma) reactions in the CANDLES experiment |
2 |
| Neutron stars with spin polarized self-interacting dark matter |
2 |
| Another step towards photodetector innovation: The first 1-inch industrial VSiPMT |
2 |
| Energy spectrum of fast second order Fermi accelerators as sources of ultra-high-energy cosmic rays |
2 |
