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[ascl:2309.013] maszcal: Mass calibrations for thermal-SZ clusters

maszcal calibrates the observable-mass relation for galaxy clusters, with a focus on the thermal Sunyaev-Zeldovich signal's relation to mass. maszcal explicitly models baryonic matter density profiles, differing from most previous approaches that treat galaxy clusters as purely dark matter. To do this, it uses a generalized Nararro-Frenk-White (GNFW) density to represent the baryons, while using the more typical NFW profile to represent dark matter.

Code site:
https://github.com/dylancromer/maszcal
Described in:
https://ui.adsabs.harvard.edu/abs/2022JCAP...10..034C
Bibcode:
2023ascl.soft09013C

Views: 405

ascl:2309.013
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