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undertake such work at ground-based solar observatories (e.g. SST or DKIST). Further, the project also likely requires collaboration with colleagues from Solar Physics and Space Plasma Research
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, structure and galaxy formation, the physics of inflation, dark matter searches and astrophysical signatures, interstellar medium physics, multi-messenger astrophysics, and investigations of black holes
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transfer, synchronization, resilient PNT, or sensing and communication systems for space, hypersonic, or GNSS-denied environments. Candidates with expertise in atomic, molecular, and optical physics
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observing programs with the James Webb Space Telescope (JWST), the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), the Sloan Digital Sky Survey (SDSS-V), the Simons Observatory, the
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-messenger astrophysics, with an anticipated start date in Fall 2027. The successful applicant will become part of the vibrant intellectual communities of the UC Berkeley Astronomy and Physics departments
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established Astraeus Space Institute, which supports space-based research across many disciplines ( https://astraeus.ufl.edu/ ). UF's world-class research facilities and telescopes
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Laboratory, which hosts the Aurora exascale supercomputer. Department members are also involved in the Kavli Institute for Cosmological Physics, the Enrico Fermi Institute, Fermilab, and Argonne
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Minimum Education: Master’s degree in Astronomy, Physics or related Physical Science subfield OR Master’s degree and 18 graduate credit hours in Astronomy, Physics, Space Science or related Physical
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OR Master’s degree and 18 graduate credit hours in Astronomy, Physics, Space Science or related Physical Science subfield. Ph.D. preferred. Minimum Experience/Training: Prior college teaching
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products and analysis procedures. They will also assist with comparing ground- and space-based observations, identifying potential data-quality issues, and preparing figures or summaries for research