Showing 1–20 of 21 results
/ Date/ Name
Jun 6, 2019Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection unitsOct 9, 2024The effect of mass loss in models of red supergiants in the Small Magellanic CloudAug 18, 2025The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population SynthesisJul 15, 2019KM3NeT front-end and readout electronics system: hardware, firmware and softwareAug 28, 2025The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversityJun 28, 2022Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASSFeb 13, 2025A new long gamma-ray burst formation pathway at solar metallicityNov 15, 2021Estimating Transient Rates from Cosmological Simulations and BPASSJun 14, 2023Observational implications of cosmologically coupled black holesAug 14, 2025White dwarf-neutron star binaries: a plausible pathway for long-duration gamma-ray bursts from compact object mergers?Aug 3, 2022VFTS 243 as predicted by the BPASS fiducial modelsAug 4, 2022New constraints on the Bray conservation-of-momentum natal kick model from multiple distinct observationsAug 23, 2024The rates and host galaxies of pair-instability supernovae through cosmic time: Predictions from BPASS and IllustrisTNGAug 28, 2025HST Deep Upper Limits Rule Out a Surviving Massive Binary Companion to the Type Ic Supernova 2012fhNov 8, 2022Can neutron star mergers alone explain the r-process enrichment of the Milky Way?Apr 15, 2026Irregularly Sampled Time Series Interpolation for Binary Evolution Simulations Using Dynamic Time WarpingOct 14, 2024Emulators for stellar profiles in binary population modelingMar 20, 2026Numerically stable equations for the orbital evolution of compact object binariesFeb 3, 2026A case for Case A: detailed look at binary black hole formation through stable mass transferJan 10, 2026A binary merger product as the direct progenitor of a Type II-P supernova