Fig. 11.

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White dwarf luminosity functions of GSPC white dwarfs within 100 pc of the Sun (red line) and spectroscopically confirmed white dwarfs within 40 pc of the Sun (blue line; McCleery et al. 2020; O’Brien et al. 2023). Error bars represent the Poisson statistics of each bolometric magnitude bin. Also shown for reference is the theoretical luminosity function from Fontaine et al. (2001) for a total age of 10 Gyr (black line).
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