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Average-atom models are an important tool in studying matter under extremeconditions, such as those conditions experienced in planetary cores, brown andwhite dwarfs, and during inertial confinement fusion. In the right context,average-atom models can yield results with similar accuracy to simulationswhich require orders of magnitude more computing time, and thus can greatlyreduce financial and environmental costs. Unfortunately, due to the wide rangeof possible models and approximations, and the lack of open-source codes,average-atom models can at times appear inaccessible. In this paper, we presentour open-source average-atom code, atoMEC. We explain the aims and structure ofatoMEC to illuminate the different stages and options in an average-atomcalculation, and to facilitate community contributions. We also discuss the useof various open-source Python packages in atoMEC, which have expedited itsdevelopment.

atoMEC: An open-source average-atom Python code