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be carried out in close collaboration with the ERC Synergy project ECOGAL (http://www.ecogal.eu/ ), of which the applicant will be a member. Currently the star formation group has three PhD students
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galaxies. The successful candidate will contribute to the exploitation of data from the GECKOS survey, a new VLT/MUSE Large Programme. GECKOS gathers deep, high spatial resolution MUSE data for 35 nearby
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as single-transit events with TESS. The successful applicant will be based at Warwick and will be responsible for scheduling observations and operating the NGTS facility, as well as planning and
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available for 3 years, from 1 April 2024. The successful candidate will ideally be in post as soon as possible, and no later than 1 October 2024. Candidates should have, or should have submitted for a PhD in
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beyond, to prepare for forthcoming surveys, such as those with the Rubin Observatory, Euclid, DESI, and Simons Observatory. The applicant should have a PhD in astronomy/astrophysics or a closely related
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have a PhD in astronomy/astrophysics or a closely related field by the starting date. Candidates are sought with experience of code development for numerical astrophysics simulations on high performance
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Experience You will hold a PhD in Astronomy, Astrochemistry or a closely related field (e.g. Physics or Chemistry). You will have prior experience working with (at least) one of the following observational
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LADUMA, MIGHTEE, and MALS, assuming leadership in coordinating data/simulation comparisons and disseminating simulation data. Additionally, the applicant would lead a robust science program, taking
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list, a statement of research plans and objectives (max 2 pages). Please also arrange for 3 reference letters to be sent to Ms Joanne Cox at j.s.cox[at]bham.ac.uk by the closing date.