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[ascl:2310.007] zCluster: Measure photometric redshifts for galaxy clusters

zCluster measures galaxy cluster photometric redshifts using data from broadband photometry in large public surveys, given a priori knowledge of the cluster position. The code retrieves and uses redshift probability distributions in order to create a projected two-dimensional density map of a targeted galaxy cluster, which is later convolved with a Gaussian kernel to smooth the map. zCluster also produces photometric redshift estimates and galaxy density maps for any point in the sky using the included zField tool.

Code site:
https://github.com/ACTCollaboration/zCluster
Used in:
https://ui.adsabs.harvard.edu/abs/2021ApJS..253....3H https://ui.adsabs.harvard.edu/abs/2021Galax...9...97P
Described in:
https://ui.adsabs.harvard.edu/abs/2018ApJS..235...20H
Bibcode:
2023ascl.soft10007H
Preferred citation method:

Please see citation information here: https://github.com/ACTCollaboration/zCluster


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ascl:2310.007
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