A Semi-Parametric Approach to Fitting Gas Pressure Profiles of Galaxy Clusters
A Semi-Parametric Approach to Fitting Gas Pressure Profiles 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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Contents
This study focuses on modelling galaxy cluster gas profiles via a semi-parametric nodal approach. While traditional methods like the generalised Navarro-Frenk-White (gNFW) often encounter parameter degeneracy, our flexible node-based method precisely defines a cluster gas pressure profile. Using Planck space telescope data from the Coma region, our...
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Full title
A Semi-Parametric Approach to Fitting Gas Pressure Profiles of Galaxy Clusters
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TN_cdi_proquest_journals_2876759193
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2876759193
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2310.07914
