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The Galaxy Cluster 'Pypeline' for X-ray Temperature Maps: ClusterPyXT

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arxiv 1903.08215 v2 pith:X3UN7M3Q submitted 2019-03-19 astro-ph.HE astro-ph.COastro-ph.GAastro-ph.IM

Brian Alden , Eric J. Hallman , David Rapetti , Jack O. Burns , Abhirup Datta This is my paper
classification astro-ph.HEastro-ph.COastro-ph.GAastro-ph.IM
keywords clusterpyxtdatax-rayclusterclustersgalaxymapsobservations
verification ladder T0 review T1 audit T2 compute T3 formal
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ClusterPyXT is a new software pipeline to generate spectral temperature, X-ray surface brightness, pressure, and density maps from X-ray observations of galaxy clusters. These data products help elucidate the physics of processes occurring within clusters of galaxies, including turbulence, shock fronts, nonthermal phenomena, and the overall dynamics of cluster mergers. ClusterPyXT automates the creation of these data products with minimal user interaction, and allows for rapid analyses of archival data with user defined parameters and the ability to straightforwardly incorporate additional observations. In this paper, we describe in detail the use of this code and release it as an open source Python project on GitHub.

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Cited by 2 Pith papers

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  1. The Treble Clef radio phoenix and its old nonthermal filaments

    astro-ph.CO 2026-07 accept novelty 6.5 of 10

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  2. The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    The magnetic field in Abell 2255 shows ordered, region-dependent orientations inferred from synchrotron intensity gradients, with radial fields in bridges and tangential fields in relics.

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