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Comparing the frequentist and Bayesian periodic signal detection: rates of statistical mistakes and sensitivity to priors. / Baluev, Roman V.
в: Monthly Notices of the Royal Astronomical Society, Том 512, № 4, 01.06.2022, стр. 5520-5534.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Comparing the frequentist and Bayesian periodic signal detection: rates of statistical mistakes and sensitivity to priors
AU - Baluev, Roman V.
PY - 2022/6/1
Y1 - 2022/6/1
N2 - We perform extensive Monte Carlo simulations to systematically compare the frequentist and Bayesian treatments of the Lomb–Scargle periodogram. The goal is to investigate whether the Bayesian period search is advantageous over the frequentist one in terms of the detection efficiency, how much if yes, and how sensitive it is regarding the choice of the priors, in particular in case of a misspecified prior (whenever the adopted prior does not match the actual distribution of physical objects). We find that the Bayesian and frequentist analyses always offer nearly identical detection efficiency in terms of their trade-off between type-I and type-II mistakes. Bayesian detection may reveal a formal advantage if the frequency prior is non-uniform, but this results in only ∼1 per cent extra detected signals. In case if the prior was misspecified (adopting non-uniform one over the actual uniform) this may turn into an opposite advantage of the frequentist analysis. Finally, we revealed that Bayes factor of this task appears rather overconservative if used without a calibration against type-I mistakes (false positives), thereby necessitating such a calibration in practice.
AB - We perform extensive Monte Carlo simulations to systematically compare the frequentist and Bayesian treatments of the Lomb–Scargle periodogram. The goal is to investigate whether the Bayesian period search is advantageous over the frequentist one in terms of the detection efficiency, how much if yes, and how sensitive it is regarding the choice of the priors, in particular in case of a misspecified prior (whenever the adopted prior does not match the actual distribution of physical objects). We find that the Bayesian and frequentist analyses always offer nearly identical detection efficiency in terms of their trade-off between type-I and type-II mistakes. Bayesian detection may reveal a formal advantage if the frequency prior is non-uniform, but this results in only ∼1 per cent extra detected signals. In case if the prior was misspecified (adopting non-uniform one over the actual uniform) this may turn into an opposite advantage of the frequentist analysis. Finally, we revealed that Bayes factor of this task appears rather overconservative if used without a calibration against type-I mistakes (false positives), thereby necessitating such a calibration in practice.
KW - methods: data analysis
KW - methods: statistical
KW - surveys
UR - https://www.mendeley.com/catalogue/99885a89-449b-33dc-9945-1df8f68ae08a/
UR - http://www.scopus.com/inward/record.url?scp=85130062707&partnerID=8YFLogxK
U2 - 10.1093/mnras/stac762
DO - 10.1093/mnras/stac762
M3 - Article
VL - 512
SP - 5520
EP - 5534
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 0035-8711
IS - 4
ER -
ID: 93468737