Unfolding X-Ray Spectral Data: Conditions and Applications

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...

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Main Authors: Sean J. Gunderson, David P. Huenemoerder
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/ad86b8
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author Sean J. Gunderson
David P. Huenemoerder
author_facet Sean J. Gunderson
David P. Huenemoerder
author_sort Sean J. Gunderson
collection DOAJ
description 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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series The Astronomical Journal
spelling doaj-art-35c0257edabd402ba317a069e156061a2024-12-03T08:19:05ZengIOP PublishingThe Astronomical Journal1538-38812024-01-011691210.3847/1538-3881/ad86b8Unfolding X-Ray Spectral Data: Conditions and ApplicationsSean J. Gunderson0https://orcid.org/0000-0003-2602-6703David P. Huenemoerder1https://orcid.org/0000-0002-3860-6230Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology , 77 Massachusetts Ave., Cambridge, MA 02139, USA ; seang97@mit.edu dph@mit.eduKavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology , 77 Massachusetts Ave., Cambridge, MA 02139, USA ; seang97@mit.edu dph@mit.eduWe 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.https://doi.org/10.3847/1538-3881/ad86b8X-ray astronomyCCD observationAstronomy data reductionSpectroscopy
spellingShingle Sean J. Gunderson
David P. Huenemoerder
Unfolding X-Ray Spectral Data: Conditions and Applications
The Astronomical Journal
X-ray astronomy
CCD observation
Astronomy data reduction
Spectroscopy
title Unfolding X-Ray Spectral Data: Conditions and Applications
title_full Unfolding X-Ray Spectral Data: Conditions and Applications
title_fullStr Unfolding X-Ray Spectral Data: Conditions and Applications
title_full_unstemmed Unfolding X-Ray Spectral Data: Conditions and Applications
title_short Unfolding X-Ray Spectral Data: Conditions and Applications
title_sort unfolding x ray spectral data conditions and applications
topic X-ray astronomy
CCD observation
Astronomy data reduction
Spectroscopy
url https://doi.org/10.3847/1538-3881/ad86b8
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AT davidphuenemoerder unfoldingxrayspectraldataconditionsandapplications