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Dr Marina Ricci (LAPP)06/06/2019, 17:30Galaxy cluster analyses at different wavelengths allows a better understanding of their formation and evolution, leading to a more realistic modeling of their physics. Comparing optical, X-ray and SZ cluster samples also enables us to check the selection functions of the surveys, and to test the cosmological representativeness of the detections. As a consequence, the multi-wavelength approach...Go to contribution page
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