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pressure conditions mimicking dense interstellar dust and molecular clouds. The applicant will use low temperature scanning tunneling microscopy (STM), temperature programmed desorption, and (single
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scanning tunneling microscopy (STM), temperature programmed desorption, and (single molecule) IR spectroscopy to follow in situ reactions leading to complex molecule formation on realistic dust grain
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preserve true structure–function relationships, and you will correlate your electrochemical findings with structural and compositional data from STM, (S)TEM, XPS, ISS, and EXAFS, feeding results back into
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