A Compound Poisson Generator approach to Point-Source Inference in Astrophysics

Abstract

The identification and description of point sources is one of the oldest problems in astronomy; yet, even today the correct statistical treatment for point sources remains one of the field's hardest problems. For dim or crowded sources, likelihood based inference methods are required to estimate the uncertainty on the characteristics of the source population. In this work, a new parametric likelihood is constructed for this problem using Compound Poisson Generator (CPG) functionals which incorporate instrumental effects from first principles. We demonstrate that the CPG approach exhibits a number of advantages over Non-Poissonian Template Fitting (NPTF) - an existing method - in a series of test scenarios in the context of X-ray astronomy. These demonstrations show that the effect of the point-spread function, effective area, and choice of point-source spatial distribution cannot, generally, be factorised as they are in NPTF, while the new CPG construction is validated in these scenarios. Separately, an examination of the diffuse-flux emission limit is used to show that most simple choices of priors on the standard parameterisation of the population model can result in unexpected biases: when a model comprising both a point-source population and diffuse component is applied to this limit, nearly all observed flux will be assigned to either the population or to the diffuse component. A new parametrisation is presented for these priors which properly estimates the uncertainties in this limit. In this choice of priors, CPG correctly identifies that the fraction of flux assigned to the population model cannot be constrained by the data.

30+10 pages, 15 figures, comments welcome; v2 updated to published version. Accompanying code available at https://github.com/ghcollin/cpg_likelihood

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Cited by in corpus (6)

• The Return of the Templates: Revisiting the Galactic Center Excess with Multi-Messenger Observations
• Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
• Extracting the gamma-ray source-count distribution below the Fermi-LAT detection limit with deep learning
• PCAT-DE: Reconstructing point-like and diffuse signals in astronomical images using spatial and spectral information
• Characterizing the Expected Behavior of Non-Poissonian Template Fitting
• On the Energy Distribution of the Galactic Center Excess' Sources