Group connectivity in COSMOS: a tracer of mass assembly history
Group connectivity in COSMOS: a tracer of mass assembly history
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Author / Creator
Darragh-Ford, E , Laigle, C , Gozaliasl, G , Pichon, C , Devriendt, J , Slyz, A , Arnouts, S , Dubois, Y , Finoguenov, A , Griffiths, R , Kraljic, K , Pan, H , Peirani, S and Sarron, F
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
Cosmic filaments are the channel through which galaxy groups assemble their mass. Cosmic connectivity, namely the number of filaments connected to a given group, is therefore expected to be an important ingredient in shaping group properties. The local connectivity is measured in COSMOS around X-Ray detected groups between redshift 0.5 and 1.2. To...
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Full title
Group connectivity in COSMOS: a tracer of mass assembly history
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TN_cdi_proquest_journals_2216559314
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2216559314
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1904.11859