A novel method for component separation of extended sources in X-ray astronomy
A novel method for component separation of extended sources in X-ray astronomy
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Ithaca: Cornell University Library, arXiv.org
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English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Contents
In high-energy astronomy, spectro-imaging instruments such as X-ray detectors allow investigation of the spatial and spectral properties of extended sources including galaxy clusters, galaxies, diffuse interstellar medium, supernova remnants and pulsar wind nebulae. In these sources, each physical component possesses a different spatial and spectra...
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Full title
A novel method for component separation of extended sources in X-ray astronomy
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TN_cdi_proquest_journals_2230481535
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2230481535
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1905.10175
