activity
20122026
most citedThe enhanced X-ray Timing and Polarimetry mission - eXTP

329 citations · 1k across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.IM2026

Soft proton experiments supporting the development of astronomical X-ray instrumentation

S. J. Diebold, B. Heß, F. Pfeifle +11

Orbital soft protons can severely degrade the performance of astronomical X-ray observatories. On the one hand, they may cause permanent radiation damage to X-ray detectors; on the…

astro-ph.IM2026

Microchannel plate detector development for ultraviolet astronomy

S. Diebold, J. Barnstedt, J. Bayer +8

Observational data from the UV wavelength range is crucial to solve several astrophysical puzzles. Consequently, there are a number of upcoming UV missions from CubeSats up to the…

astro-ph.IM2024

Quality assurance of actuators for the Medium-Sized Telescopes of the Cherenkov Telescope Array

Heiko Salzmann, Jürgen Dick, Sebastian Diebold +4

The Cherenkov Telescope Array (CTA) is a future ground-based observatory for gamma-ray astronomy providing unparalleled sensitivity in the energy range from 20 GeV up to 300 TeV. C…

astro-ph.HE2024★ 7 cited

Galactic transient sources with the Cherenkov Telescope Array Observatory

Cherenkov Telescope Array Observatory Consortium

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exh…

hep-ph2024★ 18 cited

Dark Matter Line Searches with the Cherenkov Telescope Array

S. Abe, J. Abhir, A. Abhishek +562

Monochromatic gamma-ray signals constitute a potential smoking gun signature for annihilating or decaying dark matter particles that could relatively easily be distinguished from a…

astro-ph.IM2024★ 1 cited

Using SRG/eROSITA to estimate soft proton fluxes at the ATHENA detectors

E. Perinati, M. Freyberg, M. C. H. Yeung +5

Context: Environmental soft protons have affected the performance of the X-ray detectors on board Chandra and XMM-Newton, and they pose a threat for future high energy astrophysics…