Gamma-ray bursts (GRBs) rank among the most powerful explosions in the universe, releasing immense energy in intense flashes of gamma rays. The most distant GRBs originate from the era when the first stars and galaxies formed. Detecting them allows astronomers to probe the early universe and understand how the first heavy elements formed and how the earliest stellar populations lived and died. Missions like HiZ-GUNDAM, a satellite planned for launch in the 2030s by the Japan Aerospace Exploration Agency (JAXA), aim to detect these distant explosions in real time.
However, detecting GRBs presents a major challenge. These explosions appear unpredictably across the sky, and their afterglows fade rapidly. Astronomers must therefore detect each burst quickly and determine its position immediately so that other telescopes can observe it. Wide-field X-ray monitors provide one solution, as they can observe large regions of the sky and determine the direction of incoming signals.
Some designs use lobster-eye X-ray optics, inspired by the way lobsters’ compound eyes collect light from many directions simultaneously. Yet building a single optical system from multiple lobster-eye segments and aligning them precisely remains a difficult technical task.
