Dataciencia

Colección SciELO Chile

The galaxy cluster AC114

Indexado

WoS	WOS:001235820200001
Scopus	SCOPUS_ID:85195200221

DOI

10.1051/0004-6361/202348399

Año

2024

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

The mass of a galaxy cluster appears to be a key variable in determining the importance of environmental effects in the evolution of cluster members, where massive galaxy clusters (M-vir > 10(15) M-circle dot) show changes in the slope of the MZR.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

Métricas Externas

PlumX	Altmetric	Dimensions

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Andrade, A.	-	Universidad Nacional Andrés Bello - Chile European Southern Observ - Chile European Southern Observatory Santiago - Chile
2	Saviane, Ivo	-	European Southern Observ - Chile European Southern Observatory Santiago - Chile
3	Monaco, L.	Hombre	Universidad Nacional Andrés Bello - Chile
4	Yegorova, I.	Mujer	European Southern Observ - Chile European Southern Observatory Santiago - Chile
5	Proust, Dominique	-	Observ Paris PSL - Francia GEPI - Galaxies, Etoiles, Physique, Instrumentation - Francia

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento

Fuente
European Southern Observatory under ESO

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
We thank the anonymous referee for their useful comments which improved the quality of the paper. A special thanks goes to the Dr. Piercarlo Bonifacio for the feedback presented in the early stage of this research. Additionally, we want to thanks Felipe Vivanco and Gustavo Worner, for the opportunity to discuss our results and for the valuable contributions to the development of the Python scripts used in this work. This publication is based on observations collected at the European Southern Observatory under ESO programme ID 083.A-0566. Also, this program has made use of data from the VIKING survey from VISTA at the ESO Paranal Observatory, programme ID 179.A-2004. Data processing has been contributed by the VISTA Data Flow System at CASU, Cambridge and WFAU, Edinburgh.

Agradecimiento

We thank the anonymous referee for their useful comments which improved the quality of the paper. A special thanks goes to the Dr. Piercarlo Bonifacio for the feedback presented in the early stage of this research. Additionally, we want to thanks Felipe Vivanco and Gustavo Worner, for the opportunity to discuss our results and for the valuable contributions to the development of the Python scripts used in this work. This publication is based on observations collected at the European Southern Observatory under ESO programme ID 083.A-0566. Also, this program has made use of data from the VIKING survey from VISTA at the ESO Paranal Observatory, programme ID 179.A-2004. Data processing has been contributed by the VISTA Data Flow System at CASU, Cambridge and WFAU, Edinburgh.