Galaxy cluster matter profiles I. Self-similarity, mass calibration, and observable-mass relation validation employing cluster mass posteriors

Não existem arquivos associados a este item.
Título: 
Autor(es) e Colaborador(es): 
Ludwig-Maximilians-Universitat
Max Planck Institute for Extraterrestrial Physics
Institut fur Astro- und Teilchenphysik
Laboratório Interinstitucional de e-Astronomia – LIneA
Fermi National Accelerator Laboratory
University of Michigan
Universidade Estadual Paulista (UNESP)
University of Portsmouth
University of Sussex
University College London
Instituto de Astrofisica de Canarias
The Barcelona Institute of Science and Technology
University of Trieste
INAF-Osservatorio Astronomico di Trieste
Institute for Fundamental Physics of the Universe
Universität Hamburg
IIT Hyderabad
California Institute of Technology
University of Chicago
Universidad Autonoma de Madrid
Institut d’Estudis Espacials de Catalunya (IEEC)
CSIC)
National Center for Supercomputing Applications
University of Illinois at Urbana-Champaign
Santa Cruz Institute for Particle Physics
The Ohio State University
Harvard & Smithsonian
Macquarie University
Lowell Observatory
Universidade de São Paulo (USP)
Texas A&M University
LPSC Grenoble –
Institució Catalana de Recerca i Estudis Avançats
Peyton Hall
Observatório Nacional
Northeastern University
Medioambientales y Tecnológicas (CIEMAT)
University of Southampton
Oak Ridge National Laboratory
Argonne National Laboratory
501 Campbell Hall
Lawrence Berkeley National Laboratory
Autor(es) Principais: 
Outros identificadores: 
Data: 
29-Abr-2025
1-Mar-2025
Tipo: 
Palavras-chave: 


Aparece nas coleções:Repositório Institucional - Unesp