Showing 1–20 of 30 results
/ Date/ Name
Mar 25, 2026A Fast, Hot Wind from a Nuclear StarburstFeb 13, 2026X-ray line diagnostics of the multi-phase gas in the Centaurus cluster core with XRISM/ResolveJan 23, 2026GRBAlpha, VZLUSAT-2 and GRBBeta -- GRB observations with CubeSatsOct 28, 2025XRISM constraints on unidentified X-ray emission lines, including the 3.5 keV line, in the stacked spectrum of ten galaxy clustersSep 18, 2025Stratified wind from a super-Eddington X-ray binary is slower than expectedAug 7, 2025XRISM/Resolve View of Abell 2319: Turbulence, Sloshing, and ICM DynamicsMay 10, 2025Constraining gas motion and non-thermal pressure beyond the core of the Abell 2029 galaxy cluster with XRISMNov 1, 2024Characterization of more than three years of in-orbit radiation damage of SiPMs on GRBAlpha and VZLUSAT-2 CubeSatsAug 22, 2023The cosipy library: COSI's high-level analysis softwareFeb 20, 2023GRBAlpha: the smallest astrophysical space observatory -- Part 1: Detector design, system description and satellite operationsFeb 20, 2023The peak-flux of GRB 221009A measured with GRBAlphaJul 7, 2022Early results from GRBAlpha and VZLUSAT-2Feb 16, 2021Simulations of expected signal and background of gamma-ray sources by large field-of-view detectors aboard CubeSatsJan 15, 2021The simulation framework of the timing-based localization for future all-sky gamma-ray observations with a fleet of CubesatsJul 17, 2019All-sky Medium Energy Gamma-ray Observatory: Exploring the Extreme Multimessenger UniverseJun 10, 2018CAMELOT - Concept study and early results for onboard data processing and GPS-based timestampingNov 16, 2017Hitomi Observation of Radio Galaxy NGC 1275: The First X-ray Microcalorimeter Spectroscopy of Fe-Kα Line Emission from an Active Galactic NucleusOct 12, 2017Measurements of resonant scattering in the Perseus cluster core with Hitomi SXSMay 19, 2017Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A fieldSep 2, 2015The Si/CdTe semiconductor Compton camera of the ASTRO-H Soft Gamma-ray Detector (SGD)