Showing 21–40 of 101 results
/ Date/ Name
Jun 28, 2024Initial operations of the Soft X-ray Imager onboard XRISMApr 22, 2024Squeezing the quantum noise of a gravitational-wave detector below the standard quantum limitJan 9, 2024Design study and spectroscopic performance of SOI pixel detector with a pinned depleted diode structure for X-ray astronomyNov 8, 2023TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?Oct 11, 2023Chasing Gravitational Waves with the Cherenkov Telescope ArrayOct 9, 2023Magnetic Field Properties inside the Jet of Mrk 421: Multiwavelength Polarimetry Including the Imaging X-ray Polarimetry ExplorerMay 18, 2023The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43Apr 6, 2023Spectral Type and Geometric Albedo of (98943) 2001 CC21, the Hayabusa2# Mission TargetFeb 23, 2023First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formationJan 28, 2023Surface-termination-dependent electronic states in kagome superconductors AV3Sb5 (A = K, Rb, Cs) studied by micro-ARPESJan 26, 2023Super-Resolution Analysis via Machine Learning: A Survey for Fluid FlowsDec 21, 2022JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334Dec 21, 2022Quantum repeaters: From quantum networks to the quantum internetDec 5, 2022The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 FilamentNov 23, 2022Community Engagement FrontierOct 12, 2022The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2Mar 15, 2022The International Linear Collider: Report to Snowmass 2021Jan 13, 2022B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens MainNov 18, 2021Discovery of the Fastest Early Optical Emission from Overluminous SN Ia 2020hvf: A Thermonuclear Explosion within a Dense Circumstellar EnvironmentNov 5, 2021GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run