Galaxy Cluster Matter Profiles: I. Self-similarity, Mass Calibration, and Observable-Mass Relation Validation Employing Cluster Mass Posteriors
A. Singh, J. J. Mohr, C. T. Davies,S. Bocquet,S. Grandis, M. Klein,J. L. Marshall,M. Aguena,S. S. Allam,O. Alves,F. Andrade-Oliveira,D. Bacon, S. Bhargava,D. Brooks,A. Carnero Rosell,J. Carretero, M. Costanzi,L. N. da Costa,M. E. S. Pereira,S. Desai,H. T. Diehl,P. Doel,S. Everett,B. Flaugher,J. Frieman,J. García-Bellido,E. Gaztanaga,R. A. Gruendl,G. Gutierrez,D. L. Hollowood,K. Honscheid,D. J. James,K. Kuehn,M. Lima,J. Mena-Fernández,F. Menanteau,R. Miquel,J. Myles,A. Pieres,A. K. Romer,S. Samuroff, E. Sanchez,D. Sanchez Cid,I. Sevilla-Noarbe, M. Smith,E. Suchyta,M. E. C. Swanson,G. Tarle, C. To,D. L. Tucker,V. Vikram,N. Weaverdyck,P. Wiseman OSTI OAI (US Department of Energy Office of Scientific and Technical Information)（2024）
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