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https://dspace.iiti.ac.in/handle/123456789/3754
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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Datta, Abhirup | en_US |
| dc.date.accessioned | 2022-03-17T01:00:00Z | - |
| dc.date.accessioned | 2022-03-17T15:30:07Z | - |
| dc.date.available | 2022-03-17T01:00:00Z | - |
| dc.date.available | 2022-03-17T15:30:07Z | - |
| dc.date.issued | 2019 | - |
| dc.identifier.citation | Alden, B., Hallman, E. J., Rapetti, D., Burns, J. O., & Datta, A. (2019). The galaxy cluster ‘Pypeline’ for X-ray temperature maps: ClusterPyXT. Astronomy and Computing, 27, 147-155. doi:10.1016/j.ascom.2019.04.001 | en_US |
| dc.identifier.issn | 2213-1337 | - |
| dc.identifier.other | EID(2-s2.0-85065611632) | - |
| dc.identifier.uri | https://doi.org/10.1016/j.ascom.2019.04.001 | - |
| dc.identifier.uri | https://dspace.iiti.ac.in/handle/123456789/3754 | - |
| dc.description.abstract | 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 to 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. © 2019 The Authors | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Elsevier B.V. | en_US |
| dc.source | Astronomy and Computing | en_US |
| dc.subject | Galaxies | en_US |
| dc.subject | High level languages | en_US |
| dc.subject | Open source software | en_US |
| dc.subject | Open systems | en_US |
| dc.subject | Chandra | en_US |
| dc.subject | ClusterPyXT | en_US |
| dc.subject | Galaxy clusters | en_US |
| dc.subject | Python | en_US |
| dc.subject | Software pipeline | en_US |
| dc.subject | User-defined parameters | en_US |
| dc.subject | X-ray observations | en_US |
| dc.subject | X-ray temperatures | en_US |
| dc.subject | X rays | en_US |
| dc.title | The galaxy cluster ‘Pypeline’ for X-ray temperature maps: ClusterPyXT | en_US |
| dc.type | Journal Article | en_US |
| dc.rights.license | All Open Access, Hybrid Gold, Green | - |
| Appears in Collections: | Department of Astronomy, Astrophysics and Space Engineering | |
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