Showing 1–20 of 61 results
/ Date/ Name
Jun 6, 2019Non-thermal emission from the reverse shock of the youngest galactic Supernova remnant G1.9+0.3Feb 2, 2026PRISMS. U37126, a very blue, ISM-naked starburst at z=10.255 with nearly 100% Lyman continuum escape fractionFeb 16, 2005An exceptionally bright flare from SGR1806-20 and the origins of short-duration gamma-ray burstsFeb 2, 2026PRISMS. UNCOVER-26185, a metal-poor SFG at z=10.05 with no evidence for a X-ray-luminous AGNSep 3, 2024SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejectionsFeb 20, 2009A Re-interpretation of the STEREO/STE Observations and it's ConsequencesAug 28, 2023Fast generation of Schrödinger cat states in a Kerr-tunable superconducting resonatorMar 9, 2024Precision premium transformation -- a high-precision astrometric solution based on the precision premium curveNov 16, 2003Gamma-Ray Bursts are Produced Predominately in the Early UniverseSep 26, 2013Single-shot readout of a superconducting flux qubit with a flux-driven Josephson parametric amplifierAug 24, 2021Using Gaia DR2 to make a systematic comparison between two geometric distortion solutionsOct 6, 2020Spectroscopic observation of the crossover from a classical Duffing oscillator to a Kerr parametric oscillatorJan 20, 2023Search for the decay $B^0_s \rightarrow π^0 π^0$ at BelleMay 24, 2015Critical fluctuations and the rates of interstate switching near excitation threshold of a quantum parametric oscillatorMay 13, 2011RHESSI Line and Continuum Observations of Super-hot Flare PlasmaOct 9, 2011Energy Release and Particle Acceleration in Flares: Summary and Future ProspectsMay 22, 2023Learn to Flap: Foil Non-parametric Path Planning via Deep Reinforcement LearningAug 30, 2023An Astrometric Approach to Measuring the Color of an ObjectJul 20, 2011Estimates of Densities and Filling Factors from a Cooling Time Analysis of Solar Microflares Observed with RHESSIMay 22, 2014Microwave Down-Conversion with an Impedance-Matched $Λ$ System in Driven Circuit QED