  The Disk Detective citizen science project recently released a new catalog of
disk candidates found by visual inspection of images from NASA's Wide-Field
Infrared Survey Explorer (WISE) mission and other surveys. We applied this new
catalog of well-vetted disk candidates to search for new members of nearby
young stellar associations (YSAs) using a novel technique based on Gaia data
and virtual reality (VR). We examined AB Doradus, Argus, $\beta$ Pictoris,
Carina, Columba, Octans-Near, Tucana-Horologium, and TW Hya by displaying them
in VR together with other nearby stars, color-coded to show infrared excesses
found via Disk Detective. Using this method allows us to find new association
members in mass regimes where isochrones are degenerate. We propose ten new YSA
members with infrared excesses: three of AB Doradus (HD 44775, HD 40540 and HD
44510), one of $\beta$ Pictoris (HD 198472), two of Octans-Near (HD 157165 and
BD+35 2953), and four disk-hosting members of a combined population of Carina,
Columba and Tucana-Horologium: CPD-57 937, HD 274311, HD 41992, and WISEA
J092521.90-673224.8. This last object (J0925) appears to be an extreme debris
disk with a fractional infrared luminosity of $3.7 \times 10^{-2}$. We also
propose two new members of AB Doradus that do not show infrared excesses: TYC
6518-1857-1 and CPD-25 1292. We find HD 15115 appears to be a member of
Tucana-Horologium rather than $\beta$ Pictoris. We advocate for membership in
Columba-Carina of HD 30447, CPD-35 525, and HD 35841. Finally, we propose that
three M dwarfs, previously considered members of Tuc-Hor are better considered
a separate association, tentatively called ``Smethells 165''.
