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SPEX X-ray spectral fitting package

Kaastra, J. S.; Raassen, A. J. J.; de Plaa, J.; Gu, Liyi

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    <dcat:keyword>Astrophysics</dcat:keyword>
    <dcat:keyword>Spectroscopy</dcat:keyword>
    <dcat:keyword>X-rays</dcat:keyword>
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    <dcat:keyword>Plasma</dcat:keyword>
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    <dct:description>&lt;p&gt;SPEX is a software package for fitting astrophysical X-ray spectra. It has been&amp;nbsp;developed since the 1970s at SRON Netherlands Institute for Space Research. SPEX is an&amp;nbsp;interactive command-line program for the computation of emergent spectra of optically&amp;nbsp;thin plasmas such as stellar coronal loop structures, supernova remnants (also including&amp;nbsp;transient ionization effects), photo-ionized plasmas, and optically thick plasmas. These&amp;nbsp;model spectra can be fitted to measured X-ray spectra from various X-ray observatories, like&amp;nbsp;XMM-Newton and Chandra. SPEX has been optimized for high-resolution X-ray spectroscopy, which&amp;nbsp;makes it especially suitable for analyzing grating and micro-calorimeter spectra.&amp;nbsp;&lt;/p&gt;</dct:description>
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Publication date:
August 19, 2016
DOI:
10.5281/zenodo.2222370

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Astrophysics Spectroscopy X-rays Software Plasma
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Versions

Version 3.06.00 10.5281/zenodo.3939056 Jul 10, 2020
Version 3.05.00 10.5281/zenodo.2419563 Dec 19, 2018
Version 3.04.00 10.5281/zenodo.2272992 Dec 8, 2017
Version 3.03.00 10.5281/zenodo.2246613 Nov 7, 2016
Version 3.02.00 10.5281/zenodo.2222370 Aug 19, 2016
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