# Coarse-Grained Hawkes Processes

**Authors:** Shinsuke Koyama

PMC · DOI: 10.3390/e27060555 · Entropy · 2025-05-25

## TL;DR

This paper introduces a new model for analyzing event data when only aggregated counts are available, improving accuracy and efficiency.

## Contribution

The novel coarse-grained Hawkes process model captures statistical features of aggregated event data effectively.

## Key findings

- The model accurately captures second-order statistics of bin-count data with large bin sizes.
- The proposed inference method performs as well or better than existing techniques in simulations.
- The approach maintains computational efficiency during parameter estimation.

## Abstract

When analyzing real-world event data, it is often the case that bin-count processes are observed instead of precise event time-stamps along a continuous timeline, owing to practical limitations in measurement accuracy. In this work, we propose a modeling framework for aggregated event data generated by multivariate Hawkes processes. The introduced model, termed the coarse-grained Hawkes process, effectively captures the second-order statistical characteristics of the bin-count representation of the Hawkes process, particularly when the bin size is large relative to the typical support of the excitation kernel. Building upon this model, we develop a method for inferring the underlying Hawkes process from bin-count observations, and demonstrate through simulation studies that the proposed approach performs comparably to, or even surpasses, existing techniques, while maintaining computational efficiency in parameter estimation.

## Full-text entities

- **Diseases:** infection (MESH:D007239), injury to (MESH:D014947)
- **Chemicals:** Ar (MESH:D001128)
- **Species:** Homo sapiens (human, species) [taxon 9606]

## Full text

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## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12191576/full.md

## References

29 references — full list in the complete paper: https://tomesphere.com/paper/PMC12191576/full.md

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Source: https://tomesphere.com/paper/PMC12191576