Abstract
After a review of the historical context of Bayesian inference in astronomy, we work a tutorial problem involving the search for pulsars in gamma-ray astronomical data; i.e. the detection of periodicities in a Poisson point process. We develop a model called Sparse Bayes Blocks for this purpose. These methods are also effective for estimation of the pulsar period.
This paper is followed by a commentary by statistician Eric D. Kolaczyk.
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Connors, A. (2003). Power from Understanding the Shape of Measurement: Progress in Bayesian Inference for Astrophysics. In: Statistical Challenges in Astronomy. Springer, New York, NY. https://doi.org/10.1007/0-387-21529-8_2
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DOI: https://doi.org/10.1007/0-387-21529-8_2
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