Selection effects on X-ray and strong-lensing clusters in various cosmologies
Galaxy clusters are hotter and more X-ray luminous than in quiescence while they undergo major mergers, which also transiently increase their strong-lensing efficiency. We use semi-analytic models for both effects to study how cluster dynamics in different dark-energy models affects the X-ray select...
Enregistré dans:
| Auteurs principaux: | , |
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| Format: | Article (Journal) Chapter/Article |
| Langue: | anglais |
| Publié: |
October 31, 2013
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| In: |
Arxiv
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| Accès en ligne: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/astro-ph/0703789
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| Notes sur l'auteur: | C. Fedeli and M. Bartelmann |
| Résumé: | Galaxy clusters are hotter and more X-ray luminous than in quiescence while they undergo major mergers, which also transiently increase their strong-lensing efficiency. We use semi-analytic models for both effects to study how cluster dynamics in different dark-energy models affects the X-ray selected cluster population and its strong-lensing optical depth. We find that mergers increase the number of observable X-ray clusters by factors of a few and considerably broaden their redshift distribution. Strong-lensing optical depths are increased by a very similar amount. Quite independent of cosmology, X-ray bright clusters above a flux limit of $10^{-13.5} \mathrm{erg s^{-1} cm^{-2}}$ produce $\sim60%$ of the strong-lensing optical depth, and only $\sim1%$ above a flux limit of $10^{-11.5} \mathrm{erg s^{-1} cm^{-2}}$ if mergers are taken into account. |
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| Description: | Gesehen am 25.09.2017 |
| Description matérielle: | Online Resource |