Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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The lensing signal around galaxy clusters can, in principle, be used to test detailed predictions for their average mass profile from numerical simulations. However, the intrinsic shape of the profiles can be smeared out when a sample that spans a wide range of cluster masses is averaged in physical length units. This effect especially conceals rap...
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Lensing Constraints on the Mass Profile Shape and the Splashback Radius of Galaxy Clusters
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TN_cdi_proquest_journals_2074245479
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2074245479
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1611.09366
