A single rolling grant programme will keep UK astronomers and planetary scientists at the controls of space missions like XMM-Newton and Swift, while also building the next generation of detectors and instruments for future spacecraft. The programme tackles a wide sweep of fundamental questions. In high-energy astrophysics, researchers will study gamma-ray bursts—the most powerful explosions in the universe—and the hot, violent environments around black holes and neutron stars. In planetary science, the team will model X-ray emissions from planets and test novel instruments such as the Life Marker Chip, a device designed to detect signs of past or present life on other worlds. The laboratory work pushes detector technology further, developing improved Charge Coupled Devices for future space telescopes and exploring new concepts in X-ray interferometry and polarimetry. This is primarily curiosity-driven fundamental science. There is no immediate practical application. But the detector and instrumentation work—particularly the development of more sensitive, radiation-hardened imaging sensors—has a track record of spinning off into medical imaging, security scanning, and industrial inspection. The public outreach and knowledge transfer components ensure that discoveries made at the edge of the observable universe do not stay locked inside academic journals.
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We propose a broad scientific programme encompassing astrophysics, planetary science and space intrumentation. In high energy astrophysics, we will investigate a range of phenomena including gamma-ray bursts, accretion-driven sources and high temperature galactic environments, fully utilising current missions such as XMM-Newton and Swift. Our astrophysics programme also places emphasis on dwarf stars, from hot white dwarfs through to cool dwarfs and brown dwarfs, and on exploitation of novel sky survey data from WASP and other projects. In planetary science we will further develop our expertise in modelling planetary X-ray emissions and extend our investigations of novel instrumentation, such as the Life Marker Chip, in anticipation of opportunities afforded by the Aurora and Cosmic Visions programmes. Our laboratory programme also includes the further development of Charge Coupled Device technology for application in future Space Astronomy programmes and the study of new concepts in X-ray Interferometry and X-ray Polarimetry. Finally we propose a commitment to knowledge transfer and the maintenance of a high quality and extensive public outreach activity.
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