Showing 21–40 of 1,036 results
/ Date/ Name
Feb 6, 2026Non-spherical BUFFALOs: a weak lensing view of the Frontier Field clusters and associated systematicsFeb 6, 2026The Walkaway Star HP Tau/G2: Evidence for a Stellar MergerJan 15, 2026From a Network to a Networking: The Evolution of the Latin American Giant ObservatoryDec 18, 2025The AGN nature of strong CIII emitters in the Early Universe with JWSTDec 8, 2025Searches for Light Dark Matter and Evidence of Coherent Elastic Neutrino-Nucleus Scattering of Solar Neutrinos with the LUX-ZEPLIN (LZ) ExperimentDec 8, 2025Search for Light Sterile Neutrinos With Two Neutrino Beams at MicroBooNENov 23, 2025Optimizing the potential of KM3NeT in detecting core-collapse supernovaeNov 21, 2025Search for New Physics via Low-Energy Electron Recoils with a 4.2 Tonne\times Year Exposure from the LZ ExperimentNov 21, 2025Measurements of differential charged-current cross sections on argon for electron neutrinos with final-state protons in MicroBooNENov 20, 2025Deep Learning Framework for Enhanced Neutrino Reconstruction of Single-line Events in the ANTARES TelescopeNov 17, 2025Sensitivity to low-mass WIMPs with an improved liquid argon ionization response model within the DarkSide programmeNov 17, 2025Measurement of Exclusive $π^+$--argon Interactions Using ProtoDUNE-SPNov 11, 2025Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distributionNov 10, 2025Search for steady and flaring neutrino emission from cosmic sources using the complete ANTARES datasetOct 30, 2025Baryon anti-Baryon Photoproduction Cross Sections off the ProtonOct 29, 2025Extreme equivalent width-selected low-mass starbursts at $z=4-9$: insights into their role in cosmic reionizationOct 22, 2025Quantum computation of molecular geometry via many-body nuclear spin echoesOct 20, 2025Euclid preparation: The flat-sky approximation for the clustering of Euclid's photometric galaxiesOct 17, 2025Production of radioactive $^{22}$Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observationsOct 16, 2025Measurement of $C\!P$ asymmetry in $D^0 \to K^0_{\rm S} K^0_{\rm S}$ decays with Run 3 data