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The eROSITA Final Equatorial-Depth Survey (eFEDS) – Splashback radius of X-ray galaxy clusters using galaxies from HSC survey

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Effects of multiphase gas and projection on X-ray observables in simulated galaxy clusters as seen by eROSITA

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An empirical method for mitigating an excess up-scattering mass bias on the weak lensing mass estimates for shear-selected cluster samples

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