Gamma-Ray Burst Triangulation with a Near-Earth Network

TL;DR

This paper proposes a near-Earth gamma-ray burst detection network with 9 spacecraft, capable of all-sky localization within a few degrees, using a novel ground-based localization method tested through simulations.

Contribution

It introduces a new ground processing localization method that does not depend on onboard triggers or cross-correlation, enhancing real-time GRB localization capabilities.

Findings

A 9-spacecraft network achieves several-degree localization accuracy.

The network can operate in near-real time with proper data downlink and processing.

Simulations demonstrate the effectiveness of the proposed localization method.

Abstract

We study the characteristics of Near-Earth-Networks (NENs) of gamma-ray burst (GRB) detectors, with the objective of defining a network with all-sky, full-time localization capability for multi-messenger astrophysics. We show that a minimum network consisting of 9 identical spacecraft in two orbits with different inclinations provides a good combination of sky coverage with several-degree localization accuracy with detector areas of 100 cm$^2$. In order to achieve this, careful attention must be paid to systematics. This includes accurate photon timing ($\sim$ 0.1 ms), good energy resolution ($\sim$ 10\%), and reduction of Earth albedo, which are all within current capabilities. Such a network can be scaled in both the number and size of detectors to produce increased accuracy. We introduce a new method of localization which does not rely on on-board trigger systems or on the cross-correlation of time histories, but rather, in ground processing, tests positions over the entire sky and assigns probabilities to them to detect and localize events. We demonstrate its capabilities with simulations. If the NEN spacecraft can downlink at least several hundred time- and energy-tagged events per second, and the data can be ground-processed as they are received, it can in principle derive GRB positions in near-real time over the entire sky.