High-statistics simulations of NewAthena WFI background using Geant4

Authors: Matthew Heine, Catherine E. Grant, Marshall W. Bautz et al.
Publication: Space Telescopes and Instrumentation 2026: Ultraviolet to Gamma Ray
Published: Aug 21, 2026
Source: Crossref
Back to Search View Original Cite This Article

Related Articles

Speckle correlation-based diffraction-limited high resolution polychromatic imaging through the atmospheric turbulence using the memory effect principle for a large scale telescope

Sorabh Chhabra, A. N. Ramaprakash - Aug 2026

Read More
Development of terahertz intensity interferometry for very high angular resolution studies

Hiroshi Matsuo, Hajime Ezawa et al. - Aug 2026

Read More
From reverse engineering to manufacturing: finite-element cryogenic and optomechanical validation of the GRAVITY+ SUPER HIGH-RES grism system

Alejandro S. Farah Simon, Carolina Keiman et al. - Aug 2026

Read More
MORFEO @ ELT: large-field, high-sensitivity astronomy for the ELT era

Carmelo Arcidiacono, Francesca Annibali et al. - Aug 2026

Read More
The test mass simulator (TMSim), a high precision optomechanical OGSE for LISA

Mickaël Lacroix, Jean-Christophe Barrière et al. - Aug 2026

Read More
Journal Ideas PyMinds Charcha More
PORE

About

About Us

Resources

Help Centre Research Guides CiteScore

Legal

Terms of Service Privacy Policy Cookie Policy Accessibility

Connect

Contact Us
© 2026 PORE. Content available under CC BY-NC 4.0