Future instrumentation for the study of the Warm-Hot Intergalactic Medium
F.B.S. Paerels, J.S. Kaastra, T. Ohashi, P. Richter, A.M. Bykov, J., Nevalainen
TL;DR
This paper reviews future UV and X-ray instruments needed to better understand the diffuse, highly ionised Warm-Hot Intergalactic Medium, highlighting technological requirements and scientific goals.
Contribution
It identifies key capabilities and requirements for upcoming instrumentation to study the Warm-Hot Intergalactic Medium more effectively.
Findings
Current instruments are insufficient for detailed study.
Future instrumentation needs enhanced sensitivity and resolution.
Advancements will enable new insights into intergalactic medium properties.
Abstract
We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.
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