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. Description: This research opportunity focuses on the development of the broadband THz Hot-Electron Bolometer (HEB) mixers with the ultimate sensitivity for operation on orbital and suborbital platforms
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. Description: The balance of infall and outflow of circumgalactic gas determines the long-term evolution of a galaxy, so understanding how gas gets into and out of galaxies is essential to understanding our
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available for projects related to the development and exploitation of cosmological numerical simulations and mock galaxy catalogs for weak lensing and galaxy clustering. These efforts will feed directly into
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. Description: Our research focuses on understanding basic processes which occur in solar and stellar flares through analyzing data, development of theory, and computational studies. Specifically, we are seeking
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of solar system history, recording planetary differentiation, impact flux, and volatile evolution more completely and more clearly than any other planetary body. Asteroids are fascinating worlds ranging from
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) Structure formation of the Universe and evolution of clusters of galaxies; (2) Circulation history of baryonic matter in the Universe; (3) Transport and circulation of energy in the Universe; (4) New science
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SPHEREx satellite. Likewise, data analysis on the dust lifecycle, dust composition in nearby galaxies, ice formation and evolution, Zodiacal dust, and the connections between dust and gas are possible with
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development to support extended reality technologies, machine learning pipeline integration, integration of sensors/devices to mobile platforms, and creating novel clinical decision support applications for our
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Database (Nanograindb; in development). These three databases will enable the study and interpretation of spectral signatures from carbon in the interstellar medium—including molecular clouds, planetary
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the best opportunity to understand the origin, evolution, and processes of the solar system. This opportunity is to join Dr. Yang Liu at JPL to study surface and interior processes of the parent bodies from