Semisupervised Learning for Detecting Inverse Compton Emission in Galaxy Clusters

Inverse Compton (IC) emission associated with the nonthermal component of the intracluster medium (ICM) has been a long-sought phenomenon in cluster physics. Traditional spectral fitting often suffers from the degeneracy between the two-temperature thermal (2T) spectrum and the one-temperature plus...

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Bibliographic Details
Main Authors: Sheng-Chieh Lin, Yuanyuan Su, Fabio Gastaldello, Nathan Jacobs
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad8888
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