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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 t...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2829564907

The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey

About this item

Full title

The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2023-06

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

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...

Alternative Titles

Full title

The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2829564907

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2829564907

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2306.13392

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