Two Step Localization Method for Electromagnetic Followup of LIGO-Virgo-KAGRA Gravitational-Wave Triggers

TL;DR

This paper introduces a Two-Step Localization method combining wide-field and narrow-field telescopes for rapid electromagnetic follow-up of gravitational wave events, significantly reducing detection latency through coordinated observations.

Contribution

The paper proposes a novel coordinated observational protocol that improves early EM counterpart detection efficiency compared to uncoordinated strategies.

Findings

Two-Step Localization reduces median detection latency.

Coordination significantly improves early EM detection.

Next-generation telescopes can further enhance performance.

Abstract

Rapid detection and follow-up of electromagnetic (EM) counterparts to gravitational wave (GW) signals from binary neutron star (BNS) mergers are essential for constraining source properties and probing the physics of relativistic transients. Observational strategies for these early EM searches are therefore critical, yet current practice remains suboptimal, motivating improved, coordination-aware approaches. We propose and evaluate the Two-Step Localization strategy, a coordinated observational protocol in which one wide-field auxiliary telescope and one narrow-field main telescope monitor the evolving GW sky localization in real time. The auxiliary telescope, by virtue of its large field of view, has a higher probability of detecting early EM emission. Upon registering a candidate signal, it triggers the main telescope to slew to the inferred location for prompt, high-resolution follow-up. We assess the performance of Two-Step Localization using large-scale simulations that incorporate dynamic sky-map updates, realistic telescope parameters, and signal-to-noise ratio (SNR)-weighted localization contours. For context, we compare Two-Step Localization to two benchmark strategies lacking coordination. Our results demonstrate that Two-Step Localization significantly reduces the median detection latency, highlighting the effectiveness of targeted cooperation in the early-time discovery of EM counterparts. Our results point to the most impactful next step: next-generation faster telescopes that deliver drastically higher slew rates and shorter scan times, reducing the number of required tiles; a deeper, truly wide-field auxiliary improves coverage more than simply adding more telescopes.