Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions

This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited

Detalles Bibliográficos
Autores: Brough, Sarah, Ahad, Syeda Lammim, Bahé, Yannick M., Ellien, A., Gonzalez, A. H., Jiménez-Teja, Y., Kimmig, Lucas C., Martin, Garreth, Martínez-Lombilla, C., Montes, Mireia, Pillepich, Annalisa, Ragusa, Rossella, Remus, Rhea-Silvia, Collins, Chris A., Knapen, J. H., Mihos, J. Christopher
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/372241
Acceso en línea:http://hdl.handle.net/10261/372241
Access Level:acceso abierto
Palabra clave:Galaxies: clusters: general
Galaxies: evolution
Galaxies: haloes
Galaxies: photometry
Descripción
Sumario:This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited

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