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An asteroseismic age estimate for the Pleiades using a neural-network emulator of rotating $δ$ Scuti pulsation models
Asteroseismology of $δ$ Sct stars has strong potential for determining the ages of young stars through individual mode fitting. We present a neural-network emulator trained on approximately 46 million rotating pulsation models. From stellar mass, metallicity, age, and equatorial rotation velocity, i
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