Showing 281–300 of 4,334 results
/ Date/ Name
Jun 10, 2025Euclid preparation: The NISP spectroscopy channel, on ground performance and calibrationJun 6, 2025Results from the T2K experiment on neutrino mixing including a new far detector $μ$-like sampleJun 4, 2025Experimental and simulative study on laser irradiation of 3D-printed micro-structures at intensities relevant for inertial confinement fusionJun 3, 2025Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early UniverseJun 3, 2025Measurement of the branching fractions of the Cabibbo-favored decays $Λ_{c}^{+}\toΛK_{S}^{0}K^{+}$ and $Λ_{c}^{+}\toΞ^{0}K_{S}^{0}π^{+}$ and search for $Λ_{c}^{+}\toΣ^{0} K_{S}^{0}K^{+}$Jun 2, 2025Science Prospects for the Southern Wide-field Gamma-ray Observatory: SWGOMay 29, 2025Exploring the keV-scale physics potential of CUOREMay 29, 2025The ambiguous AT2022rze: Changing-look AGN mimicking a supernova in a merging galaxy systemMay 28, 2025First measurement of neutron capture multiplicity in neutrino-oxygen neutral-current quasi-elastic-like interactions using an accelerator neutrino beamMay 23, 2025Betelgeuse, Betelgeuse, Betelgeuse, Betel-buddy? Constraints on the dynamical companion to $α$ Orionis from HSTMay 23, 2025Betelgeuse's Buddy: X-Ray Constraints on the Nature of $α$ Ori BMay 23, 2025The NEXT-100 DetectorMay 20, 2025Searching for Light Dark Matter and Dark Sectors with the NA64 experiment at the CERN SPSMay 16, 2025Unbound neutron $\nu0d_{3/2}$ strength in $^{17}$C and the N=16 shell gapMay 16, 2025EMU/GAMA: A new approach to characterising radio luminosity functionsMay 15, 2025Origin of the ring ellipticity in the black hole images of M87*May 14, 2025Three regimes of a picosecond magnetoacoustics in ferromagnetic structuresMay 14, 2025Asteroid sizes determined with thermophysical model and stellar occultationsMay 12, 2025Measurement of the Total Compton Scattering Cross Section between 6.5 and 11 GeVMay 9, 2025The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies