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Can Radiative Cooling and Nongravitational Heating Explain Simultaneously the Global X‐Ray Properties of Clusters and the Unresolved Cosmic X‐Ray Background?

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Measuring Feedback Using the Intergalactic Medium State and Evolution Inferred from the Soft X‐Ray Background

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Autocorrelation Function of the Soft X‐Ray Background Produced by Warm‐Hot Gas in Dark Halos

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