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Table 1.

Stellar, disk, and accretion properties for the targets in the Upper Scorpius region.

Name Disk Dist SpT Teff AV L log Lacc M acc Acc? Mdisk, dust
type [pc] [K] [mag] L L M M yr−1 M
2MASSJ15534211-2049282 Full 136 ± 4 M4 3270 1.2 0.09 −2.6 0.24 3.66 × 10−10 Y 1.69 × 10−06
2MASSJ15583692-2257153 Full 166 ± 4 K0 5110 0.0 2.57 −0.5 1.63* 1.59 × 10−08 Y 1.51 × 10−04
2MASSJ16001844-2230114 Full 138 ± 9 M4.5 3200 0.8 0.08 −1.9 0.20 2.03 × 10−09 Y 2.31 × 10−06
2MASSJ16035767-2031055 Full 143 ± 1 K6 4205 0.7 0.48 −1.8 0.91 8.81 × 10−10 Y 2.74 × 10−06
2MASSJ16035793-1942108 Full 158 ± 2 M2 3560 0.3 0.13 −5.1 0.42 6.69 × 10−13 N 9.16 × 10−07
2MASSJ16041740-1942287 Full 161 ± 2 M3 3415 0.7 0.14 −4.3 0.31 6.04 × 10−12 N 7.26 × 10−07
2MASSJ16041893-2430392 ... 145 M2 3560 0.3 0.45 −3.1 0.37 1.48 × 10−10 Y ...
2MASSJ16042165-2130284 Transitional 150 ± 1 K3 4730 1.4 0.90 −3.2 1.24 3.09 × 10−11 N 1.55 × 10−04
2MASSJ15354856-2958551_E Full (binary) 145 M4.5 3200 0.0 0.10 −2.8 0.20 3.53 × 10−10 Y 1.27 × 10−06
2MASSJ15354856-2958551_W ... (binary) 145 M4.5 3200 0.0 0.10 −2.9 0.20 2.73 × 10−10 Y 1.27 × 10−06
2MASSJ15514032-2146103 Evolved 142 ± 2 M4.5 3200 0.3 0.05 −3.5 0.19 5.01 × 10−11 Y 4.82 × 10−07
2MASSJ15530132-2114135 Full 146 ± 2 M4.5 3200 0.8 0.05 −3.0 0.19 1.52 × 10−10 Y 3.88 × 10−06
2MASSJ15582981-2310077 Full 147 ± 3 M4.5 3200 1.0 0.05 −2.3 0.19 7.16 × 10−10 Y 4.00 × 10−06
2MASSJ16014086-2258103 Full 145 M3 3415 1.2 0.12 −1.2 0.31 7.42 × 10−09 Y 2.28 × 10−06
2MASSJ16020757-2257467 Full 140 ± 1 M2 3560 0.4 0.08 −3.8 0.44 1.08 × 10−11 Y 3.25 × 10−06
2MASSJ16024152-2138245 Full 142 ± 2 M5.5 3060 0.6 0.03 −2.9 0.12 2.76 × 10−10 Y 6.46 × 10−06
2MASSJ16054540-2023088 Full 145 ± 2 M4.5 3200 0.6 0.10 −2.8 0.20 3.58 × 10−10 Y 5.05 × 10−06
2MASSJ16062196-1928445 Transitional 145 M1 3705 0.8 0.34 −1.3 0.46 6.13 × 10−09 Y 2.69 × 10−06
2MASSJ16063539-2516510 Evolved 139 ± 3 M4.5 3200 0.0 0.03 −5.1 0.18 8.62 × 10−13 N 1.03 × 10−06
2MASSJ16064385-1908056 Evolved 144 ± 7 K7 4060 0.4 0.29 −2.3 0.82 2.65 × 10−10 Y 5.48 × 10−07
2MASSJ16072625-2432079 Full 143 ± 2 M3 3415 0.7 0.18 −2.6 0.29 4.56 × 10−10 Y 8.39 × 10−06
2MASSJ16081566-2222199 Full 140 ± 2 M2 3560 0.5 0.15 −3.7 0.41 1.99 × 10−11 N 5.98 × 10−07
2MASSJ16082324-1930009 Full 138 ± 1 M0 3850 1.1 0.32 −2.0 0.61 7.90 × 10−10 Y 2.58 × 10−05
2MASSJ16082751-1949047 Evolved 145 M5.5 3060 0.6 0.06 −3.1 0.14 1.97 × 10−10 Y 5.01 × 10−07
2MASSJ16090002-1908368 Full 139 ± 3 M4.5 3200 0.3 0.05 −4.2 0.19 1.02 × 10−11 Y 1.05 × 10−06
2MASSJ16090075-1908526 Full 138 ± 1 M0 3850 1.0 0.32 −1.7 0.60 1.74 × 10−09 Y 2.81 × 10−05
2MASSJ16095361-1754474 Full 158 ± 5 M4.5 3200 0.5 0.04 −4.5 0.18 4.54 × 10−12 Y 6.78 × 10−07
2MASSJ16104636-1840598 Full 143 ± 3 M4.5 3200 1.2 0.04 −3.9 0.19 1.45 × 10−11 Y 1.14 × 10−06
2MASSJ16111330-2019029 Full 155 ± 1 M3.5 3340 0.6 0.03 −1.9 0.27 9.77 × 10−10 Y 3.69 × 10−06
2MASSJ16123916-1859284 Full 139 ± 2 M1 3705 0.6 0.22 −2.3 0.50 4.75 × 10−10 Y 3.65 × 10−06
2MASSJ16133650-2503473 Full 145 M3 3415 1.0 0.11 −1.6 0.32 2.93 × 10−09 Y 5.80 × 10−07
2MASSJ16135434-2320342 Full 145 M4.5 3200 0.3 0.12 −2.3 0.20 1.18 × 10−09 Y 4.97 × 10−06
2MASSJ16141107-2305362 Full 145 K4 4590 0.3 1.05 −1.4 1.25 2.09 × 10−09 Y 3.15 × 10−06
2MASSJ16143367-1900133 Full 142 ± 2 M3 3415 1.9 0.52 −2.7 0.29 5.17 × 10−10 Y 7.84 × 10−07
2MASSJ16154416-1921171 Full 132 ± 2 K7 4060 2.8 0.30 −0.3 0.81 2.44 × 10−08 Y 1.28 × 10−05
2MASSJ16181904-2028479 Evolved 138 ± 2 M5 3125 1.6 0.05 −3.4 0.16 8.05 × 10−11 Y 2.76 × 10−06

Notes. Disk type from Barenfeld et al. (2016), Luhman & Mamajek (2012), Carpenter et al. (2006). Stellar properties obtained using the Baraffe et al. (2015) evolutionary models, apart from the target 2MASSJ15583692-2257153, for which Siess et al. (2000) models were used since the stellar mass was higher than the maximum one modeled by Baraffe et al. (2015). Disk masses are updated from Barenfeld et al. (2016) using the distance inferred from the Gaia DR2 (Gaia Collaboration 2018) parallaxes. When no uncertainties on the distance is reported, the mean distance to the targets of 145 pc was adopted. Possible non-accretors are reported with “N” in the Acc? column. The values reported here for the accretion rate of non-accretors are considered in this work as upper limits.

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