Showing 21–40 of 117 results
/ Date/ Name
Oct 11, 2023Chasing Gravitational Waves with the Cherenkov Telescope ArraySep 7, 2023Prospects for $γ$-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope ArraySep 1, 2023Comparing recent PTA results on the nanohertz stochastic gravitational wave backgroundAug 7, 2023Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and VirgoJul 25, 2023The NANOGrav 12.5-year Data Set: Search for Gravitational Wave MemoryJun 28, 2023The NANOGrav 15-year Gravitational-Wave Background MethodsJun 28, 2023The NANOGrav 15-year Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole BinariesJun 28, 2023The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave BackgroundJun 28, 2023The NANOGrav 15-Year Data Set: Detector Characterization and Noise BudgetJun 28, 2023The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave BackgroundMar 31, 2023Workflows Community Summit 2022: A Roadmap RevolutionOct 27, 2022The Gaia-ESO survey: mapping the shape and evolution of the radial abundance gradients with open clustersJun 6, 2022The Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacyMar 22, 2022Quality Control of Mass-Produced GEM Detectors for the CMS GE1/1 Muon UpgradeJan 3, 2022All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 dataNov 30, 2021All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 dataNov 5, 2021GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing RunOct 25, 2021Dancing in the void: hydrodynamical N-body simulations of the extremely metal poor galaxy DDO 68Oct 4, 2021Comparative case study of two methods to assess the eruptive potential of selected active regionsSep 24, 2021Search for subsolar-mass binaries in the first half of Advanced LIGO and Virgo's third observing run