Experimental K-shell x-ray and EUV spectra from charge exchange collisions of Ar18+ and O8+ ions with neutrals in an EBIT, compared to multichannel Landau-Zener models.
Athena+: The first Deep Universe X-ray Observatory
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abstract
The Advanced Telescope for High-energy Astrophysics (Athena+) is being proposed to ESA as the L2 mission (for a launch in 2028) and is specifically designed to answer two of the most pressing questions for astrophysics in the forthcoming decade: How did ordinary matter assemble into the large scale structures we see today? and how do black holes grow and shape the Universe? For addressing these two issues, Athena+ will provide transformational capabilities in terms of angular resolution, effective area, spectral resolution, grasp, that will make it the most powerful X-ray observatory ever flown. Such an observatory, when opened to the astronomical community, will be used for virtually all classes of astrophysical objects, from high-z gamma-ray bursts to the closest planets in our solar neighborhood. In this paper, we briefly review the core science objectives of Athena+, present the science requirements and the foreseen implementation of the mission, and illustrate its transformational capabilities compared to existing facilities.
fields
physics.atom-ph 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
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X-ray and extreme-ultraviolet spectra from collisions of Ar$^{18+}$ and O$^{8+}$ ions with neutrals
Experimental K-shell x-ray and EUV spectra from charge exchange collisions of Ar18+ and O8+ ions with neutrals in an EBIT, compared to multichannel Landau-Zener models.