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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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{
  "publisher": "Zenodo", 
  "DOI": "10.5281/zenodo.2222370", 
  "language": "eng", 
  "title": "SPEX X-ray spectral fitting package", 
  "issued": {
    "date-parts": [
      [
        2016, 
        8, 
        19
      ]
    ]
  }, 
  "abstract": "<p>SPEX is a software package for fitting astrophysical X-ray spectra. It has been&nbsp;developed since the 1970s at SRON Netherlands Institute for Space Research. SPEX is an&nbsp;interactive command-line program for the computation of emergent spectra of optically&nbsp;thin plasmas such as stellar coronal loop structures, supernova remnants (also including&nbsp;transient ionization effects), photo-ionized plasmas, and optically thick plasmas. These&nbsp;model spectra can be fitted to measured X-ray spectra from various X-ray observatories, like&nbsp;XMM-Newton and Chandra. SPEX has been optimized for high-resolution X-ray spectroscopy, which&nbsp;makes it especially suitable for analyzing grating and micro-calorimeter spectra.&nbsp;</p>", 
  "author": [
    {
      "family": "Kaastra, J. S."
    }, 
    {
      "family": "Raassen, A. J. J."
    }, 
    {
      "family": "de Plaa, J."
    }, 
    {
      "family": "Gu, Liyi"
    }
  ], 
  "version": "3.02.00", 
  "type": "article", 
  "id": "2222370"
}
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