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Table 2

Disk fractions from this work and the literature in various regions.

References Disk fraction (%) SpT range Mass rangea (MJup) Region Ageb (Myr) Nobjects d Method
This work 37.5 ± 6.2 6–11.8 Upper Sco 5 32 W1–W2 vs Mass
37.56.2+3.1$37.5_{ - 6.2}^{ + 3.1} $ 11.8–16.8 5 32
34.2 ± 0.0 16.8–25 5 38
38.57.7+7.7$38.5_{ - 7.7}^{ + 7.7} $ 8–13.7 10 24
25.90.0+7.4$25.9_{ - 0.0}^{ + 7.4} $ 13.7–15.5 10 27
32.1 ± 3.6 15.5–25 10 28

Luhman & Esplin (2020) 233+4$23_{ - 3}^{ + 4} $ M8–L2 10.5–36.7 Upper Sco 10 27/115 Ks –I2/W2 vs SpT
Luhman (2025) 26 M6.25–M9.5 14.8–97.8 Upper Sco 10 52/200 W1–W2 vs SpT
Luhman et al. (2016) 52 ± 10 M8–L0 10.6–23 NGC 1333 3 11/21 Literature (Spitzer)
Scholz et al. (2023) 4216+18$42_{ - 16}^{ + 18} $ M9–L3 5.9–12.0 NGC 1333 2 5/12 K–I2 vs SpT
Esplin & Luhman (2019) 417+8$41_{ - 7}^{ + 8} $ M8–L0 14.2–23.7 Taurus 3 15/37 Ks –I2/W2 vs SpT
Damian et al. (2023) 80 ± 55 c 10.5–32.5 σ Orionis 2–3 5/6 Ks–W2 slope
Luhman et al. (2016) 429+11$42_{ - 9}^{ + 11} $ M8–L0 10.6–23 IC 348 3 10/24 Literature (Spitzer)
Seo & Scholz (2025) 4612+13$46_{ - 12}^{ + 13} $ M9–L1 9.3–13.2 IC 348 3 6/13 K–IRAC2 vs SpT + SED modeling

Notes. a Mass range when not explicitly given in the referenced study, inferred using the Faherty et al. (2016) temperature scale for young brown dwarfs and the evolutionary models of Saumon & Marley (2008), based on the spectral type and the ageb of the region. b Age of the region as adopted by the authors. Note that these values may differ across studies and may have been revised in light of recent constraints, particularly following the release of Gaia data (e.g., Gaia DR2 and DR3; Gaia Collaboration 2018, 2021). c Not shown in Fig. 7 to preserve clarity due to its extreme value and ill-defined error. d Number of objects in each mass bin for this study. Fractions expressed as Ndisk/Ntot represent those found in the literature values, as reported by the authors. Fields marked with “–” indicate values not specified by the authors.

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