The miniJPAS survey: Cluster and galaxy group detections with AMICO
[Context] Samples of galaxy clusters allow us to better understand the physics at play in galaxy formation and to constrain cosmological models once the mass, position (for clustering studies), and redshift are known. In this context, large optical datasets play a crucial role.
| Autores: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2023 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/350447 |
| Acceso en línea: | http://hdl.handle.net/10261/350447 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxies: clusters: general Galaxies: evolution Galaxies: luminosity function, mass function |
| Sumario: | [Context] Samples of galaxy clusters allow us to better understand the physics at play in galaxy formation and to constrain cosmological models once the mass, position (for clustering studies), and redshift are known. In this context, large optical datasets play a crucial role. |
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