G Ponti, X Zheng, N Locatelli, S Bianchi… - Astronomy & …, 2023 - aanda.org
Context. Despite their vital importance to understanding galaxy evolution and our own Galactic ecosystem, our knowledge of the physical properties of the hot X-ray emitting phase …
M Barbera, A Argan, E Bozzo… - Journal of Low …, 2016 - Springer
ATHENA is the L2 mission selected by ESA to pursue the science theme “Hot and Energetic Universe.” One of the two focal plane instruments is the X-ray Integral Field Unit, an array of …
M Barbera, UL Cicero, L Sciortino… - … 2018: Ultraviolet to …, 2018 - spiedigitallibrary.org
The X-ray Integral Field Unit (X-IFU) is one of the two instruments of the Athena astrophysics space mission approved by ESA in the Cosmic Vision 2015-2025 Science Programme. The …
B Cabrera - Journal of Low Temperature Physics, 2008 - Springer
Abstract Superconducting Transition Edge sensors (TES) devices are now in use across a broad range of applications including dark matter searches, gamma ray and x-ray …
We present here a combined analysis of four high spectral resolution observations of the Diffuse X-ray Background, made using the University of Wisconsin-Madison/Goddard Space …
We present a measurement of the K-shell spectrum from highly charged xenon ions recorded with a high-energy x-ray calorimeter spectrometer array that can distinguish …
Lyman x-ray spectra following charge exchange between C 6+ and H 2 are presented for collision velocities between 400 and 2300 km/s (1–30 keV/amu). Spectra were measured by …
RT Zhang, DG Seely, VM Andrianarijaona… - The Astrophysical …, 2022 - iopscience.iop.org
Laboratory measurements of X-ray emissions following charge exchange (CX) between highly charged ions and neutrals are important to assess their diagnostic utility for the …
X-ray spectra following charge-exchange collisions between C 6+ and He are presented for collision energies between 460 and 32 000 eV/u. Spectra were obtained at the Oak Ridge …