Showing 161–180 of 7,941 results
/ Date/ Name
Jan 7, 2026Detector characterization for a new $^{12}$C+$^{12}$C reaction study at LUNAJan 7, 2026Modelling spacecraft-emitted electrons measured by SWA-EAS experiment on board Solar Orbiter missionJan 6, 2026Differential cross sections for ${{^{12}\mathrm{C}(n,α_{0})}}$, ${{^{16}\mathrm{O}(n,α_{0})}}$ and ${{^{16}\mathrm{O}(n,α_{1,2,3})}}$ between ${E_n}$ = 7.2 and 10 MeV with an active-target Time Projection ChamberJan 5, 2026A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematicsJan 4, 2026Simulation of the CYGNO Gaseous TPC Optical ReadoutJan 4, 2026Hilbert space signatures of non-ergodic glassy dynamicsJan 2, 2026About the origin of the magnetic ground state of Tb$_{2}$Ir$_{2}$O$_{7}$Jan 1, 2026KMT-2024-BLG-0816/OGLE-2024-BLG-0519 -- A Microlensing Event with Candidate Free-Floating Planet Lens and Blended LightDec 30, 2025Understanding Solar Flares and Energetic Events: Open questions, observational requirements, and instrumental needs over the coming decadeDec 30, 2025Picture an Astronomer: Best Practices for Retaining Talent in AstrophysicsDec 30, 2025Fast reconstruction-based ROI triggering via anomaly detection in the CYGNO optical TPCDec 24, 2025Atomic clock frequency ratios with fractional uncertainty $\leq 3.2 \times 10^{-18}$Dec 24, 2025Observation of disorder-induced superfluidityDec 23, 2025Alfvénic solar wind intervals observed by Solar Orbiter: Exploiting the capability of the SWA plasma suite and source region investigationDec 22, 2025Ultra-high precision high voltage system for PTOLEMYDec 22, 2025Nuclear Physics Mid Term Plan at LNGSDec 19, 2025Constraining the Prompt Atmospheric Neutrino Flux Combining IceCube's Cascade and Track SamplesDec 19, 2025Improved $S$-factor of the $^{13}$C(p,$γ$)$^{14}$N reaction at $E_{\mathrm{p}}\,=\,$330-740 keV and parameters of resonances at 448 keV and 551 keVDec 18, 2025Cygnus X-3: A variable petaelectronvolt gamma-ray sourceDec 18, 2025The AGN nature of strong CIII emitters in the Early Universe with JWST