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Atomic Data Needs for Modeling Photoionized Plasmas
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Many of the fundamental questions in astrophysics can be addressed using spectroscopic observations of photoionized cosmic plasmas. However, the reliability of the inferred astrophysics depends on the accuracy of the underlying atomic data used to interpret the collected spectra. In this paper, we review some of the most glaring atomic data needs for better understanding photoionized plasmas.
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Rate coefficients for dielectronic recombination of N-like Ne
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