Stellar age compression in spectroscopic estimates can produce apparent rapid thick-disk formation signatures without requiring an intrinsically bursty history.
Deep learning of multi-element abundances from high-resolution spectroscopic data
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Stellar Age Compression Reshapes Interpretations of the Milky Way Thick-Disk Formation History
Stellar age compression in spectroscopic estimates can produce apparent rapid thick-disk formation signatures without requiring an intrinsically bursty history.