Objective Bayesian analysis of "on/off" measurements
Diego Casadei

TL;DR
This paper develops an objective Bayesian approach for analyzing low-count 'on/off' measurements in astrophysics, providing a more accurate inference method that accounts for uncertainties and is valid across different count regimes.
Contribution
It introduces a Bayesian solution based on the reference posterior for 'on/off' measurements and compares it with existing methods, enhancing inference accuracy for faint sources.
Findings
Bayesian method performs well at low counts where asymptotic approximations fail.
Proposed significance calculation accounts for background uncertainty.
Comparison shows advantages over traditional asymptotic significance formulas.
Abstract
In high-energy astrophysics, it is common practice to account for the background overlaid with the counts from the source of interest with the help of auxiliary measurements carried on by pointing off-source. In this "on/off" measurement, one knows the number of photons detected while pointing to the source, the number of photons collected while pointing away of the source, and how to estimate the background counts in the source region from the flux observed in the auxiliary measurements. For very faint sources, the number of detected photons is so low that the approximations which hold asymptotically are not valid. On the other hand, the analytical solution exists for the Bayesian statistical inference, which is valid at low and high counts. Here we illustrate the objective Bayesian solution based on the reference posterior and compare the result with the approach very recently…
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