Unfolding X-Ray Spectral Data: Conditions and Applications

Abstract We present conditions for which X-ray spectra can be “unfolded” to present an accurate representation of the true source spectra. The method we use to unfold the data is implemented in the Interactive Spectral Interpretation Software and distinguishes itself as being model-independent. We find that this method of unfolding makes accurate representations of the true source spectra: (1) The detector is high-resolution, and (2) The spectrum is not steeply sloped. These criteria are not simple conditions that give concrete determinations; each detector and spectrum must be judged individually. We find that both grating and imaging detectors can be unfolded with minimal distortions as compared to both continuum and local spectral features, the latter CCD detectors being much more energy dependent. We also provide example use cases for unfolding in the context of current generation X-ray observatories and important caveats.

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Publication Details

Journal
The Astronomical Journal
Published
2024-12-03
DOI
https://doi.org/10.3847/1538-3881/ad86b8
Citations
2
Primary Topic
Statistical and numerical algorithms
Type
article
Field-Weighted Citation Impact
1.95

Funders

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article

Unfolding X-Ray Spectral Data: Conditions and Applications

Sean J. Gunderson, David P. Huenemoerder
2 citations
The Astronomical Journal
Statistical and numerical algorithms
1.95
article

Unfolding X-Ray Spectral Data: Conditions and Applications

Sean J. Gunderson, David P. Huenemoerder
article en
2 citations

Abstract

Abstract We present conditions for which X-ray spectra can be “unfolded” to present an accurate representation of the true source spectra. The method we use to unfold the data is implemented in the Interactive Spectral Interpretation Software and distinguishes itself as being model-independent. We find that this method of unfolding makes accurate representations of the true source spectra: (1) The detector is high-resolution, and (2) The spectrum is not steeply sloped. These criteria are not simple conditions that give concrete determinations; each detector and spectrum must be judged individually. We find that both grating and imaging detectors can be unfolded with minimal distortions as compared to both continuum and local spectral features, the latter CCD detectors being much more energy dependent. We also provide example use cases for unfolding in the context of current generation X-ray observatories and important caveats.

The Astronomical JournalVol. 169(1)
Massachusetts Institute of Technology (US)
Smithsonian Astrophysical Observatory
Affordable and clean energy
Openalex Percentile: Top 13%
Statistical and numerical algorithms
1.95
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