Showing 61–80 of 4,334 results
/ Date/ Name
Mar 2, 2026Measurement of the $e^+e^-\toπ^+π^-π^0$ cross section in the energy region from 0.56 to 1.1 GeV with the SND detectorFeb 28, 2026First Amplitude Analysis of $D^0\rightarrow K^-π^0e^+ν_e$ and Observation of $D^0\rightarrow K^*_2(1430)^-e^+ν_e$Feb 27, 2026Design of a high voltage delivery system for noble liquid time projection chambersFeb 26, 2026Neutrino NSI in archaeological PbFeb 24, 2026Low-Energy Radon Backgrounds from Electrode Grids in Dual-Phase Xenon TPCsFeb 18, 2026Measurement of the Muon Flux at the Sanford Underground Research Facility with the LUX-ZEPLIN Dark Matter DetectorFeb 17, 2026The COHERENT Experiment: 2026 UpdateFeb 13, 2026LHAASO observation of Mrk 421 during 2021 March - 2024 March: a comprehensive VHE catalog of multi-timescale outbursts and its time average behaviorFeb 13, 2026TIC65910228b: A single-transit discovery of a massive long-period warm Jupiter with TESSFeb 12, 2026Semantic-aware Adversarial Fine-tuning for CLIPFeb 11, 2026Constraints on dark axion portal: missing energy and fermion EDMsFeb 6, 2026First results from the E302 efficiency$\unicode{x2013}$instability experiment at the FACET-II facilityFeb 3, 2026The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812Feb 2, 2026Unraveling the Brown Dwarf Desert: Four New Discoveries and a Unifying, Period-Coded PictureFeb 2, 2026Mitigating half-wave plate systematics at the map-making level: calibration requirements for LiteBIRDFeb 2, 2026PRISMS. U37126, a very blue, ISM-naked starburst at z=10.255 with nearly 100% Lyman continuum escape fractionJan 29, 2026Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERISJan 29, 2026The Little Blue and Red Dots Rosetta Stones: Non-Gaussian broad lines, hot dust, and X-ray weaknessJan 29, 2026The $^{8}$Be nucleus and the Hoyle state in dissociation of relativistic nucleiJan 28, 2026Performance of the Particle-Identification Silicon-Telescope Array Coupled with the VAMOS++ Magnetic Spectrometer