Shot noise in clustering power spectra

We show that the ‘shot noise’ bias in angular clustering power spectra observed from discrete samples of points is not noise, but rather a known additive contribution that naturally arises due to degenerate pairs of points. In particular, we show that the true shot noise contribution cannot have a ‘non-Poissonian’ value, even though all point processes with non-trivial two-point statistics are non-Poissonian. Apparent deviations from the ‘Poissonian’ value can arise when significant correlations or anti-correlations are localised on small spatial scales. However, such deviations always correspond to a physical difference in two-point statistics, not a difference in noise. In the context of simulations, if clustering is treated as the tracer of a discretised underlying density field, any sub- or super-Poissonian sampling of the tracer induces such small-scale modifications and vice versa; we show this explicitly using recent innovations in angular power spectrum estimation from discrete catalogues. Finally, we show that the full covariance of clustering power spectra can also be computed explicitly: it depends only on the two-, three- and four-point statistics of the point process. The usual Gaussian covariance approximation appears as one term in the shot noise contribution, which is non-diagonal even for Gaussian random fields and Poisson sampling.

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Publication Details

Journal
The Open Journal of Astrophysics
Published
2025-10-14
DOI
https://doi.org/10.33232/001c.145919
Citations
1
Primary Topic
Neural Networks and Applications
Type
article
Field-Weighted Citation Impact
2.48
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article

Shot noise in clustering power spectra

Alex D. Hall, N Tessore
1 citations
The Open Journal of Astrophysics
Neural Networks and Applications
2.48
article

Shot noise in clustering power spectra

Alex D. Hall, N Tessore
article en
1 citations

Abstract

We show that the ‘shot noise’ bias in angular clustering power spectra observed from discrete samples of points is not noise, but rather a known additive contribution that naturally arises due to degenerate pairs of points. In particular, we show that the true shot noise contribution cannot have a ‘non-Poissonian’ value, even though all point processes with non-trivial two-point statistics are non-Poissonian. Apparent deviations from the ‘Poissonian’ value can arise when significant correlations or anti-correlations are localised on small spatial scales. However, such deviations always correspond to a physical difference in two-point statistics, not a difference in noise. In the context of simulations, if clustering is treated as the tracer of a discretised underlying density field, any sub- or super-Poissonian sampling of the tracer induces such small-scale modifications and vice versa; we show this explicitly using recent innovations in angular power spectrum estimation from discrete catalogues. Finally, we show that the full covariance of clustering power spectra can also be computed explicitly: it depends only on the two-, three- and four-point statistics of the point process. The usual Gaussian covariance approximation appears as one term in the shot noise contribution, which is non-diagonal even for Gaussian random fields and Poisson sampling.

The Open Journal of AstrophysicsVol. 8
University College London (GB), University of Edinburgh (GB)
Openalex Percentile: Top 8%
Neural Networks and Applications
2.48
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