The baryon mass function for galaxy clusters
Context. The evolution of the cluster abundance with redshift is known to be a powerful cosmological constraint when applied to X-ray clusters. Recently, the evolution of the baryon mass function has been proposed as a new variant that is free of the uncertainties present in the temperature-mass rel...
Guardado en:
| Autores principales: | Nuza, S.E., Blanchard, A. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v452_n1_p47_Nuza |
| Aporte de: |
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