Non-thermal emission from galaxy clusters
C. Ferrari (1) ((1) UNS, CNRS, OCA, Laboratoire Cassiop\'ee, Nice,, France)
TL;DR
This paper discusses the significance of non-thermal emission studies in galaxy clusters and emphasizes the importance of combining future radio survey data with WFXT observations.
Contribution
It highlights the potential of integrating radio and X-ray data for advancing understanding of non-thermal processes in galaxy clusters.
Findings
Non-thermal emissions are crucial for galaxy cluster studies.
Combining radio and X-ray data enhances analysis capabilities.
Future surveys will improve detection of non-thermal phenomena.
Abstract
The relevance of non-thermal cluster studies and the importance of combining observations of future radio surveys with WFXT data are discussed in this paper.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsRadio Astronomy Observations and Technology · Astronomical Observations and Instrumentation · Astronomy and Astrophysical Research