An Improved Atlas of Full-scan Spectra from ISO/SWS

Abstract We present an atlas of full-scan spectra from the Short-Wavelength Spectrometer (SWS) on board the Infrared Space Observatory after reprocessing and improving an earlier version published 22 yr ago. The SWS spectra cover the wavelength range from 2.35 to 45.3 μ m. They include scans in 12 separate bands, and we have updated the methods used to combine those bands into a single continuous spectrum. The main improvement comes from applying multiple constraints, including new photometry and spectra from the Infrared Spectrograph on the Spitzer Space Telescope that have become available since the release of the original products, and individualized attention to each spectrum, to renormalize the separate bands into a more consistent single spectrum. In particular, this removed unphysical negative fluxes that were common in the original data products. The new database, with 1035 reprocessed spectra, will be available to the community at NASA’s Infrared Science Archive, which also hosts the original processing.

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Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2025-09-22
DOI
https://doi.org/10.3847/1538-4365/adf848
Primary Topic
CCD and CMOS Imaging Sensors
Type
article
Field-Weighted Citation Impact
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article

An Improved Atlas of Full-scan Spectra from ISO/SWS

G. C. Sloan, T. A. Kuchar, D. R. Mizuno, K. E. Kraemer et al.
The Astrophysical Journal Supplement Series
CCD and CMOS Imaging Sensors
article

An Improved Atlas of Full-scan Spectra from ISO/SWS

G. C. Sloan, T. A. Kuchar, D. R. Mizuno, K. E. Kraemer, S. Greene, E.R. Cohen, Holly Branco
article en

Abstract

Abstract We present an atlas of full-scan spectra from the Short-Wavelength Spectrometer (SWS) on board the Infrared Space Observatory after reprocessing and improving an earlier version published 22 yr ago. The SWS spectra cover the wavelength range from 2.35 to 45.3 μ m. They include scans in 12 separate bands, and we have updated the methods used to combine those bands into a single continuous spectrum. The main improvement comes from applying multiple constraints, including new photometry and spectra from the Infrared Spectrograph on the Spitzer Space Telescope that have become available since the release of the original products, and individualized attention to each spectrum, to renormalize the separate bands into a more consistent single spectrum. In particular, this removed unphysical negative fluxes that were common in the original data products. The new database, with 1035 reprocessed spectra, will be available to the community at NASA’s Infrared Science Archive, which also hosts the original processing.

The Astrophysical Journal Supplement SeriesVol. 280(2)
Boston College (US), University of North Carolina at Chapel Hill (US), Space Telescope Science Institute (US), Georgia Institute of Technology (US), Université Bourgogne Franche-Comté (FR), Embry–Riddle Aeronautical University (US)
Openalex Percentile: Top 75%
CCD and CMOS Imaging Sensors
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An Improved Atlas of Full-scan Spectra from ISO/SWS — G. C. Sloan, T. A. Kuchar, et al. · The Astrophysical Journal Supplement Series (2025) | TGRS Research Map | TGRS