Showing 1–20 of 52 results
/ Date/ Name
Jun 11, 2021High-resolution Laboratory Measurements of K-shell X-ray Line Polarization and Excitation Cross Sections in Heliumlike S XV IonsMar 29, 2022Helium-like X-ray line complexes show that the hottest plasma on the O supergiant zeta Puppis is in its windNov 15, 2018Perspectives on Astrophysics Based on Atomic, Molecular, and Optical (AMO) TechniquesJul 5, 2010Modeling broadband X-ray absorption of massive star windsApr 25, 2011Chandra X-ray spectroscopy of the very early O supergiant HD 93129A: constraints on wind shocks and the mass-loss rateSep 28, 2010X-ray spectral diagnostics of activity in massive starsJan 16, 2024High-Precision Transition Energy Measurements of Neon-like Fe XVII IonsNov 21, 2017Glimpse of the highly obscured HMXB IGR J16318-4848 with HitomiOct 6, 2006Evidence for the importance of resonance scattering in X-ray emission line profiles of the O star $ζ$ PuppisDec 6, 2007Quantitative analysis of resolved X-ray emission line profiles of O starsAug 27, 2021Fe XVII $2p$-$3s$ line ratio diagnostic of shock formation radius in O starsJan 7, 2018In-flight Calibration of Hitomi Soft X-ray Spectrometer (3) Effective AreaSep 5, 2002X-ray spectroscopy of Eta Carinae with XMM-NewtonDec 25, 2023High count rate effects in event processing for XRISM/Resolve x-ray microcalorimeterMay 20, 2025Comprehensive Laboratory Benchmark of K-shell Dielectronic Satellites of Fe XXV-XXI IonsMar 12, 2020Observation of strong two-electron--one-photon transitions in few-electron ionAug 14, 2025Benchmark of the Fe XXV R ratio in photoionized plasma during eclipse of Centaurus X-3 with XRISM/ResolveFeb 13, 2024Laboratory Benchmark of $n\geq4$ Dielectronic Recombination Satellites of Fe XVIIJan 22, 2022New Measurement Resolves Key Astrophysical Fe XVII Oscillator Strength ProblemJun 16, 2020Chandra spectral measurements of the O supergiant $ζ$ Puppis indicate a surprising increase in the wind mass-loss rate over 18 years