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Poisson vs. Gaussian statistics for sparse X-ray data: Application to the soft X-ray spectrometerReliable results when fitting X-ray data require proper consideration of the statistics
involved. We probe the impact of Gaussian versus Poisson statistics at low count levels using both the standard χ^(2) method and maximum likelihood based on Poisson (C) statistics. The difference is studied and quantified through simulated spectra with known properties. We then test the results through analysis of Mn Kα calibration data taken with the flight spare microcalorimeter for the Hitomi soft X-ray spectrometer. Through comparison with simulations, our results show that the χ^(2) method tends to give overly optimistic estimates of the detector energy resolution, in particular when there are few counts. Given an energy resolution of ∼5 eV and a line with about 100 photons, the line width becomes ∼10% lower in the χ^(2) method than in Poisson statistics. This is a consequence of the uncertainties being dominated by counting statistics, and therefore highlights the need to choose the appropriate fit statistic.
Document ID
20210013161
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Shinya Yamada
(Tokyo Metropolitan University Tokyo, Tôkyô, Japan)
Magnus Axelsson
(Tokyo Metropolitan University Tokyo, Tôkyô, Japan)
Yoshitaka Ishisaki
(Tokyo Metropolitan University Tokyo, Tôkyô, Japan)
Saori Konami
(Tokyo Metropolitan University Tokyo, Tôkyô, Japan)
Nozomi Takemura
(Tokyo Metropolitan University Tokyo, Tôkyô, Japan)
Richard L Kelley
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Caroline A Kilbourne ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Maurice A Leutenegger
(Goddard Space Flight Center Greenbelt, Maryland, United States)
F Scott Porter
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Megan E Eckart
(Lawrence Livermore National Laboratory Livermore, California, United States)
Andrew Szymkowiak
(Yale University New Haven, Connecticut, United States)
Date Acquired
April 5, 2021
Publication Date
July 19, 2019
Publication Information
Publication: Publications of the Astronomical Society of Japan
Publisher: Oxford University Press
Volume: 71
Issue: 4
Issue Publication Date: August 1, 2019
ISSN: 0004-6264
e-ISSN: 2053-051X
URL: https://academic.oup.com/pasj/article/71/4/75/5536242
Subject Category
Astronomy
Funding Number(s)
WBS: 888692
CONTRACT_GRANT: JSPS KAKENHI 16H02190
CONTRACT_GRANT: JSPS KAKENHI 15H05438
CONTRACT_GRANT: JSPS KAKENHI 18H03714
CONTRACT_GRANT: JSPS KAKENHI 18H05458
CONTRACT_GRANT: DE-AC52-07NA27344
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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