Fig. 1.

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Steps required to run the NN on-sky. First, training data is collected using the internal source by applying random shapes on the DM and recording the resulting PWFS images. After that, the NN is trained on these data and is converted to an optimized TensorRT engine. This engine is loaded in the MagAO-X control software and runs in real time, picking up the PWFS image stream and writing to the mode coefficient stream.
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