Showing 501–520 of 6,054 results
/ Date/ Name
Jan 3, 2025Effects of Galaxy Cluster Structure on Lensed Gravitational WavesJan 2, 2025Exploiting Application-to-Architecture Dependencies for Designing Scalable OSDec 31, 2024Angular differential and elemental fragmentation cross sections of a $400\,\text{MeV/nucleon}$ $^{16}\text{O}$ beam on a graphite target with the FOOT experimentDec 28, 2024Demographics of black holes at $<$100 R$_{\rm g}$ scales: accretion flows, jets, and shadowsDec 27, 2024Measurement of the hard exclusive $π^{0}$ muoproduction cross section at COMPASSDec 27, 2024DeepSeek-V3 Technical ReportDec 25, 2024Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experimentDec 19, 2024Phase consistency test to identify type II strongly lensed gravitational wave signals using a single eventDec 18, 2024Demonstrating dynamic surface codesDec 18, 2024Measurement of the branching fraction and $\it CP$-violating asymmetry of the decay $B^{0} \rightarrow π^{0} π^{0}$ using $387$ million bottom-antibottom meson pairs in Belle II dataDec 18, 2024Scaling and logic in the color code on a superconducting quantum processorDec 12, 2024Two Earth-size Planets and an Earth-size Candidate Transiting the Nearby Star HD 101581Dec 10, 2024Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak LensingDec 10, 2024Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic techniqueDec 9, 2024A multi-technique detection of an eccentric giant planet around accelerating star HD 57625Dec 8, 2024Hydrogen Ionization Inside the SunDec 6, 2024Performance of the prototype beam drift chamber for LAMPS at RAON with proton and Carbon-12 beamsDec 6, 2024Observation of Cosmic-Ray Anisotropy in the Southern Hemisphere with 12 yr of Data Collected by the IceCube Neutrino ObservatoryDec 6, 2024First constraint for atmospheric millicharged particles with the LUX-ZEPLIN experimentDec 5, 2024CO-to-H$_2$ conversion factor and grain size distribution through the analysis of $α_\mathrm{CO}$-$q_\mathrm{PAH}$ relation