Multi-messenger Astronomy: a Bayesian approach
G. Torralba Elipe, R. A. Vazquez, E. Zas

TL;DR
This paper introduces a Bayesian framework for integrating diverse multi-messenger astronomical data, enabling comprehensive analysis of high-energy cosmic phenomena using measurements from various observational channels.
Contribution
It presents a novel Bayesian method for combining multi-messenger data, incorporating theoretical models and experimental measurements for improved astrophysical insights.
Findings
Feasibility demonstrated through simulations
Method effectively combines data from different messengers
Supports analysis of high-energy cosmic events
Abstract
After the discovery of the gravitational waves and the observation of neutrinos of cosmic origin, we have entered a new and exciting era where cosmic rays, neutrinos, photons and gravitational waves will be used simultaneously to study the highest energy phenomena in the Universe. Here we present a fully Bayesian approach to the challenge of combining and comparing the wealth of measurements from existing and upcoming experimental facilities. We discuss the procedure from a theoretical point of view and using simulations, we also demonstrate the feasibility of the method by incorporating the use of information provided by different theoretical models and different experimental measurements.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Pulsars and Gravitational Waves Research
