Weekly Working Hours: 37
Fixed Term Contract: End Date: 30 September 2026
Welsh Language: Not Applicable
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About the Role
The position is being offered until the end of September 2026, however, an extension beyond this date will be considered if the expected external project funding allows nearer the time.
The Centre for Electronic Imaging (CEI) is a research centre based within the School of Physical Sciences at the Open University. The CEI is a collaboration between the Open University and Teledyne e2v, a world-leading manufacturer of scientific and industrial image sensors. The CEI is dedicated to conducting research into advanced imaging technologies for science applications and conducts its research in collaboration with many universities, agencies and companies including the UK Space Agency, European Space Agency (ESA), NASA and Teledyne e2v.
A main focus for the CEI is the development and characterisation of detectors for space missions. One such mission is the Habitable Worlds Observatory (HWO), NASA's next flagship space telescope. Current designs for HWO have a 6-8m main mirror, with instruments covering the ultraviolet (UV), optical and near-infrared wavelengths. The main science goal of HWO is the direct detection of life on other planets, and for this purpose, it will carry a broad instrument suite including a coronograph, a high-resolution imager, and a multi-object spectrograph.
The CEI is working with several UK and international research institutions, including NASA/JPL, on the development, testing, and verification of the performance of the UV-enhanced CMOS image sensors (CIS) towards implementing these as possible detectors for one or more instruments for HWO.
We are seeking a motivated and capable individual with relevant physics, engineering and/or laboratory experience to join the CEI Habitable Worlds Observatory (HWO) project team as a Space Detector Calibration Engineer. The role will be focused on the testing and space qualification of UV-enhanced CMOS Image Sensors (CIS) for the HWO mission. As part of the CEI HWO team, the candidate will receive the necessary training to work within the CEI laboratories and will be involved in all stages of detector development and characterisation, including planning and executing calibration test campaigns and performance simulations, with the goal of optimising detector functionality for flight. The work will be closely aligned with the science requirements of UV astronomy, ensuring a strong connection between instrument performance and mission objectives.
The role involves close collaboration with colleagues at the Open University and a broad network of national and international partners. The successful candidate will engage with external collaborators across the HWO programme, including NASA/JPL, the University of Leicester, Mullard Space Science Laboratory, RAL Space, and the UK Astronomy Technology Centre, among others. Key responsibilities will include attending project meetings and international conferences, preparing and delivering technical progress reports, and maintaining active communication with both engineering and scientific teams throughout the HWO collaboration.
In addition, the role holder will have the opportunity to be involved in a variety of other research projects across the CEI, including other space missions and mission concepts for ESA (e.g. Euclid, SMILE, Theseus, X-ray interferometry) and NASA (e.g. the Nancy Grace Roman Space Telescope).
Key Responsibilities
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