The probability of identifying the cosmic web environment of galaxies around clusters motivated by t...
The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey
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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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Upcoming wide-field spectroscopic surveys will observe galaxies in a range of cosmic web environments in and around galaxy clusters. In this paper, we test and quantify how successfully we will be able to identify the environment of individual galaxies in the vicinity of massive galaxy clusters, reaching out to \(\sim5R_{200}\) into the clusters' i...
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The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey
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TN_cdi_proquest_journals_2829564907
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2829564907
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2306.13392