Showing 21–40 of 381 results
/ Date/ Name
Nov 7, 2025Precise Measurement of the Cosmic Ray Helium Spectrum above 0.1 PeVNov 6, 2025Massive stars exploding in a He-rich circumstellar medium XII. SN 2024acyl: A fast, linearly declining Type Ibn supernova with early flash-ionisation featuresOct 27, 2025First detection of ultra-high energy emission from gamma-ray binary LS I +61 303Oct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 16, 2025Measurement of $C\!P$ asymmetry in $D^0 \to K^0_{\rm S} K^0_{\rm S}$ decays with Run 3 dataOct 14, 2025Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadowOct 10, 2025Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and ForecastsOct 9, 2025Identification of low-energy kaons in the ProtoDUNE-SP detectorOct 7, 2025Study of few-electron backgrounds in the LUX-ZEPLIN detectorSep 18, 2025Low-energy nuclear recoil calibration of the LUX-ZEPLIN experiment with a photoneutron sourceSep 9, 2025Towards mono-energetic virtual $ν$ beam cross-section measurements: A feasibility study of $ν$-Ar interaction analysis with DUNE-PRISMSep 6, 2025Operation of a Modular 3D-Pixelated Liquid Argon Time-Projection Chamber in a Neutrino BeamSep 3, 2025Search for low-mass electron-recoil dark matter using a single-charge sensitive SuperCDMS-HVeV DetectorAug 27, 2025Euclid: A machine-learning search for dual and lensed AGN at sub-arcsec separationsAug 26, 2025Flow-dependent tagging of $^{214}$Pb decays in the LZ dark matter detectorAug 4, 2025Low-Energy Calibration of SuperCDMS HVeV Cryogenic Silicon Calorimeters Using Compton StepsJul 24, 2025SVOM GRB 250314A at z $\simeq$ 7.3: an exploding star in the era of reionizationJul 17, 2025Einstein Probe Discovery of EP J182730.0-095633: A New Black Hole X-ray Binary Candidate in Faint Outburst?Jul 11, 2025Spatial and Temporal Evaluations of the Liquid Argon Purity in ProtoDUNE-SPJul 10, 2025Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390