Gamma Ray Bursts in the Era of Rapid Followup
C.G. Mundell (1), C. Guidorzi (2), I.A. Steele (1) (on behalf of, the Liverpool GRB team) ((1) ARI, Liverpool John Moores University, (2), Physics Department, University of Ferrara)

TL;DR
This paper discusses advancements in gamma-ray burst research enabled by rapid robotic optical telescopes, highlighting new software, instrumentation, and scientific insights gained from prompt multi-wavelength observations.
Contribution
It introduces innovative real-time analysis software and novel instrumentation for early-time observations, advancing understanding of GRB physics in the rapid follow-up era.
Findings
Real-time automatic analysis of GRB light curves
Unique early-time polarization measurements
Enhanced understanding of GRB physics through rapid multi-wavelength data
Abstract
We present a status report on the study of gamma-ray bursts (GRB) in the era of rapid follow-up using the world's largest robotic optical telescopes - the 2-m Liverpool and Faulkes telescopes. Within the context of key unsolved issues in GRB physics, we describe (1) our innovative software that allows real-time automatic analysis and interpretation of GRB light curves, (2) the novel instrumentation that allows unique types of observations (in particular, early time polarisation measurements) and (3) the key science questions and discoveries to which robotic observations are ideally suited, concluding with a summary of current understanding of GRB physics provided by combining rapid optical observations with simultaneous observations at other wavelengths.
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