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              <text>The Marsh Observatory is a new on-campus astronomical observatory that opened in November 2023, equipped with a 0.4m robotic telescope capable of imaging planets, stars, and galaxies. Our project aims to explore new scientific applications for the Marsh Observatory and test it's observational limits using the main telescope, as well as developing and implementing a new solar telescope system to enable continuous imaging of the Sun.</text>
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              <text>This project explores the possibility of using CAR-T therapy to treat allergies. A CAR-T receptor specific to IgE antibodies was designed, a plasmid containing the receptor was created and this was expressed in Jurkat T cells. An activation assay confirmed that these cells were activated in the presence of the IgE Fc region. This CAR-T receptor may therefore be used for further research as it could be able to specifically target and kill B cells expressing IgE.</text>
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              <text>The Marsh Observatory at the University of Warwick is highly dependent on specific weather conditions to operate effectively, often leading to the postponement of key activities such as outreach events and astrophysics research. Observatories worldwide are unique in their design, geographical location, and operating environments, meaning they often require bespoke solutions to address site-specific challenges. Common issues such as dew formation, cloud cover, and high wind speeds are primary causes of dome closure. Addressing these limitations has the potential to significantly improve observatory uptime and overall performance. Relevant sensors will be installed within the observatory dome to measure ambient temperature and humidity, followed by computational analysis to determine an appropriate feedback response to changing environmental conditions. This data, alongside principles from applied thermodynamics, will inform the design specifications of the dew heater. In parallel, a custom “flat panel” will be prototyped to explore the possibility of capturing essential calibration frames under unfavourable weather conditions. The current use of an air conditioning unit to provide uniform heating across the dome results in significant energy waste and can impede overall telescope image quality. By implementing a more localised heating solution, energy usage can be reduced while minimising thermal disturbances around the optical system. This leads to improved image quality and increased thermal efficiency, both of which enhances observatory performance. This research and development will provide a framework for other institutional observatories to replicate and implement similar upgrades within their own systems, offering a more cost-effective and efficient solution to these observational challenges.</text>
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