On the same Gaia 40 parsec white dwarf sample, the luminosity function, absolute G magnitude distribution, and direct age methods give star formation histories that agree within systematic uncertainties.
A., Bruzual G., D \' az-Gonz \'a lez D
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Comparison of methods used to derive the Galactic star formation history from white dwarf samples
On the same Gaia 40 parsec white dwarf sample, the luminosity function, absolute G magnitude distribution, and direct age methods give star formation histories that agree within systematic uncertainties.