Showing 1–20 of 42 results
/ Date/ Name
Mar 26, 2026Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing runMar 19, 2026GWTC-4.0: Tests of General Relativity. I. Overview and General TestsJan 7, 2026Detector characterization for a new $^{12}$C+$^{12}$C reaction study at LUNAOct 27, 2025Towards a comprehensive study of the 14N(p,g)15O astrophysical key reaction: Description of the experimental technique including novel target preparationOct 2, 2025Status and future directions for direct cross-section measurements of the 13C(a,n)16O reaction for astrophysicsSep 4, 2025GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave PropagationAug 25, 2025GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing RunJul 16, 2025All-sky search for long-duration gravitational-wave transients in the first part of the fourth LIGO-Virgo-KAGRA Observing runMay 28, 2025Improved direct measurement of low-energy resonances in the $^{21}$Ne(p,$γ$)$^{22}$Na reactionFeb 19, 2025A Comparative Analysis of R-Matrix Fitting: ${}^{12}$C$(p,γ)$${}^{13}$N as Test CaseJan 24, 2025Humanity's Last ExamNov 7, 2024Characterization of the LUNA neutron detector array for the measurement of the 13C(a,n)16O reactionJun 3, 2024CHEOPS in-flight performance: A comprehensive look at the first 3.5 years of operationsFeb 4, 2024Constraints on Triton atmospheric evolution from occultations: 1989-2022Nov 7, 2023First measurement of the low-energy direct capture in 20Ne(p, γ)21Na and improved energy and strength of the Ecm = 368 keV resonanceAug 30, 2023New proton-capture rates on carbon isotopes and their impact on the astrophysical $^{12}\mathrm{C}/{}^{13}\mathrm{C}$ ratioAug 7, 2023Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and VirgoApr 11, 2023Detector signal characterization with a Bayesian network in XENONnTSep 7, 2022First direct limit on the 334 keV resonance strength in the $^{22}$Ne(α,γ)$^{26}$Mg reactionMar 4, 2022A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics