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Table D.1

Comparison sample.

Identifier D (pc) Group Age (Myr) SpT L* (L) M* (M) Td (K) Ldisk/L* Rdisk (au) Wdisk (au) L12CO (W m−2) MCO (M) Refs. Label
RZ Psc 184.7 . . . 30±10 G8V 0.80 1.10 500 7.0e-02 6.0 . . . <3.23×1016 <1.0 × 10−5 43 . . .
49 Cet 57.1 ARG 48±10 A2V 15.61 1.95 155/56 2.0e-04/7.0e-04 136.0 147.0 1.16±0.12×1018 7.11.1+1.2$\[7.1_{-1.1}^{+1.2}\]$ × 10−3 2,22,26,30,48 a
HD 15115 48.7 THA 37±11 F4V 3.60 1.40 62 5.1e-04 93.0 21.0 <4.80×1015 <1.2×10−6 17,22,35,36,48 . . .
HD 15745 71.5 BPMG 21±4 F0V 4.20 1.40 147/81 3.5e-04/1.9e-03 65.0 <50.0 <4.71×1016 <1.2×10−5 10,22,24 . . .
HD 21997 69.6 COL 36±8 A4V 10.49 1.76 61 5.7e-04 94.0 52.0 9.15±0.93×1017 4.80.9+0.8$\[4.8_{-0.9}^{+0.8}\]$ × 10−2 2,22,26,48 b
HD 32297 129.3 . . . <30 A7V 7.98 1.65 234/82 8.7e-04/6.2e-03 122.3 62.0 1.58±0.15×1018 5.01.5+1.6$\[5.0_{-1.5}^{+1.6}\]$ × 10−2 1,2,16,22,30,48 c
HD 36546 99.9 118TAU 10±3 A2V 13.86 1.86 570/135 . . ./4.0e-03 70.0 150.0 2.45±0.25×1018 3.21.2+1.2$\[3.2_{-1.2}^{+1.2}\]$ × 10−3 13,22,37,48 d
β Pic 19.4 BPMG 21±4 A6V 8.65 1.75 85 2.6e-03 105.0 92.0 1.58±0.18×1017 4.81.4+1.2$\[4.8_{-1.4}^{+1.2}\]$ × 10−5 2,4,11,21,22,38,47 e
HD 48370 35.9 COL 36±8 K0V 0.77 0.96 41 5.6e-04 88.3 37.1 <4.01×1016 <1.2×10−5 2,20,28,36 . . .
HD 61005 36.4 ARG 48±10 G8Vk 0.64 0.92 109/52 2.9e-04/3.0e-03 72.6 38.0 <1.05×1016 <4.0×10−6 1,2,22,36 . . .
HD 95086 86.4 CAR 28±11 A8V 6.55 1.58 184/54 1.5e-04/1.3e-03 206.0 180.0 <1.43×1016 <4.0×10−6 2,19,22,26,48 f
HD 98363 137.0 LCC 15±3 A4V 12.02 1.83 295/112 2.8e-04/6.4e-04 . . . . . . <6.22×1016 <9.5×10−6 3,29,48 . . .
HD 106906 102.2 LCC 15±3 F5V 7.02 2.71 108/53 1.5e-03/3.5e-04 100.0 80.0 <3.84×1016 <8.3×10−6 1,10,22,34,40,48 . . .
HR 4796 70.7 TWA 10±3 A0V 21.42 2.10 108 4.6e-03 77.8 14.8 <4.60×1016 <3.5×10−6 9,10,22,39,48 g
HD 109832 107.1 LCC 15±3 F1V 5.37 1.46 186/92 2.5e-04/5.1e-04 . . . . . . <3.49×1016 <6.4×10−6 1,19,29,48 . . .
HD 110058 129.7 LCC 15±3 A5V 8.71 1.67 499/112 2.4e-05/1.4e-03 30.9 48.9 1.41±0.18×1017 9.32.2+3.5$\[9.3_{-2.2}^{+3.5}\]$ × 10−3 2,3,6,48 h
HD 111161 109.2 LCC 15±3 A5V 9.05 1.68 142 7.2e-04 71.3 . . . <4.61×1016 <1.2×10−5 8,12,48 i
HD 111520 107.8 LCC 15±3 F5/6V 2.66 1.32 107/45 1.4e-03/1.5e-03 76.0 50.0 <5.13×1016 <1.3×10−5 1,12,22,36,48 . . .
HD 112810 133.2 LCC 15±3 F3/5V 3.54 1.36 227/58 1.9e-04/1.1e-03 90.0 <200.0 <6.86×1016 <1.8×10−5 1,12,22,34,48 . . .
HD 113556 100.3 LCC 15±3 F2V 4.42 1.41 268/60 8.9e-05/4.4e-04 110.0 <400.0 <3.33×1016 <8.5×10−6 3,12,22,36,48 . . .
HD 113766 108.6 LCC 15±3 F3/5V 4.00 1.50 490/15 3.3e-02/7.0e-04 30.0 <60.0 <4.88×1016 <1.3×10−5 12,22,33,34,42,48 . . .
HD 114082 94.9 LCC 15±3 F3V 3.75 1.47 110 4.3e-03 38.0 <40.0 <1.66×1016 <4.9×10−6 1,10,22,36 . . .
HD 115600 108.9 LCC 15±3 F2V 4.75 1.48 109 2.5e-03 90.0 <200.0 <4.58×1016 <1.2×10−5 1,12,22,48 . . .
HD 117214 107.1 LCC 15±3 F6V 5.35 1.50 111 3.1e-03 42.0 <50.0 <2.11×1016 <5.2×10−6 1,10,22,48 . . .
HD 121191 131.9 LCC 15±3 A7V 7.58 1.62 555/118 2.1e-03/2.6e-03 55.0 54.0 3.43±0.34×1017 5.62.8+3.3$\[5.6_{-2.8}^{+3.3}\]$ × 10−3 2,10,22,29,44,48 j
HD 121617 117.5 UCL 16±2 A2V 14.51 1.90 105 4.8e-03 78.0 60.0 1.61±0.17×1018 2.60.4+0.5$\[2.6_{-0.4}^{+0.5}\]$ × 10−2 2,22,25,29,48 k
HD 129590 135.9 UCL 16±2 G3V 3.00 1.30 89 7.7e-03 79.0 70.0 9.51±2.38×1016 9.56.5+6.5$\[9.5_{-6.5}^{+6.5}\]$ × 10−5 1,10,22 x
HD 131488 151.4 UCL 16±2 A2V 13.64 1.87 570/94 2.8e-03/2.7e-03 92.0 46.0 1.64±0.17×1018 9.31.2+1.2$\[9.3_{-1.2}^{+1.2}\]$ × 10−2 22,29,44,48 1
HD 131835 129.1 UCL 16±2 A4V 9.81 1.72 176/71 8.2e-04/2.2e-03 83.7 87.0 1.22±0.13×1018 1.60.3+0.2$\[1.6_{-0.3}^{+0.2}\]$ × 10−2 2,12,22,27,48 m
HD 134888 111.8 UCL 16±2 F3/5V 3.27 1.36 166/67 3.0e-04/1.0e-03 . . . . . . <6.90×1016 <1.8×10−5 1,12,48 . . .
HD 135953 127.3 UCL 16±2 F5V 2.42 1.22 61 9.0e-04 . . . . . . <8.05×1016 <2.1×10−5 1,12,48 . . .
HD 138813 135.9 US 10±3 A1V 21.74 2.11 153/75 7.4e-04/7.4e-04 120.0 130.0 2.39±0.27×1018 2.00.4+0.4$\[2.0_{-0.4}^{+0.4}\]$ × 10−2 12,22,46,48 n
HD 141569 111.3 . . . 5.90.6+1.9$\[5.9_{-0.6}^{+1.9}\]$ A0Ve 21.88 2.06 . . . 9.0e-03 130.0 240.0 1.14±0.11×1019 1.00.2+0.5$\[1.0_{-0.2}^{+0.5}\]$ × 10−1 5,23,45 o
HD 142446 135.0 UCL 16±2 F3V 3.73 1.39 239/65 1.8e-04/7.7e-04 110.0 80.0 <9.05×1016 <2.3×10−5 1,12,22,48 . . .
NO Lup 132.8 Lupus 1–3 K7 0.29 0.70 117/12025$\[117 /_{120}^{25-}\]$ 3.4e-03/4.0e032.0e07$\[3.4 \mathrm{e}\text{-}03 /_{4.0 \mathrm{e}-03}^{2.0 \mathrm{e}-07-}\]$ <56.0 . . . 7.06±1.70×1017 4.91.1+1.1$\[4.9_{-1.1}^{+1.1}\]$ × 10−5 7,14,15 . . .
HD 143675 135.0 UCL 16±2 A7V 8.40 1.67 374/127 1.8e-04/4.1e-04 52.4 . . . <1.68×1016 <5.0×10−6 3,8,10,29,48 p
HD 145263 141.2 US 10±3 F2V 4.98 1.50 265 1.5e-02 . . . . . . <1.05×1017 <2.7×10−5 12,32,34,48 . . .
HD 145560 120.8 UCL 16±2 F5V 3.27 1.35 103/53 1.8e-03/2.1e-03 76.0 50.0 <4.43×1016 <1.1×10−5 1,12,22,48 . . .
HD 145880 123.0 UCL 16±2 A0V 19.74 2.06 196/70 2.9e-04/8.3e-04 . . . . . . <9.88×1016 <2.0×10−5 1,19,29,48 . . .
HD 146181 127.0 UCL 16±2 F6V 2.81 1.28 124/71 9.6e-04/2.0e-03 74.0 <90.0 <5.34×1016 <1.4×10−5 1,12,22,36,48 . . .
HD 146897 131.6 US 10±3 F2/3V 4.78 1.42 304/94 3.0e-04/5.3e-03 82.0 <90.0 9.57±2.39×1016 4.01.5+59.1$\[4.0_{-1.5}^{+59.1}\]$ × 10−5 2,3,12,22,48 y
HD 156623 108.0 UCL 16±2 A2V 13.28 1.86 605/123 1.6e-03/3.4e-03 77.8 119.0 1.27±0.13×1018 2.10.4+0.4$\[2.1_{-0.4}^{+0.4}\]$ × 10−3 12,19,29,48 q
HD 172555 28.8 BPMG 21±4 A7V 7.84 1.66 250 7.5e-04 7.5 . . . 1.30±0.23×1016 8.33.8+3.8$\[8.3_{-3.8}^{+3.8}\]$ × 10−6 41,42,48 r
HD 181327 47.7 BPMG 21±4 F6V 2.83 1.41 78 2.6e-03 81.3 16.0 6.49±1.13×1015 1.90.6+1.9$\[1.9_{-0.6}^{+1.9}\]$ × 10−6 2,18,22,35,36 z
HD 191089 50.0 BPMG 21±4 F5V 2.73 1.20 92 1.5e-03 44.8 16.0 <1.15×1016 <2.9×10−6 10,22,35,36 . . .
CP-72 2713 36.7 BPMG 21±4 K7Ve 0.19 0.80 43 1.1e-03 130.0 100.0 <2.68×1016 <6.9×10−6 22,31,36,48 . . .

Notes. With the exception of β Pic, whose distance data are from the Hipparcos catalog (van Leeuwen 2007), the distance estimates are from Bailer-Jones et al. (2021) using their geometric approach that is based only on the Gaia EDR3 parallaxes. Group membership information is based on the BANYAN Σ model (Gagné et al. 2018) in most cases, while for HD 48370 and NOLup are from Torres et al. (2008) and Lovell et al. (2021a), respectively. For stars known to be members of stellar associations, we have adopted the ages of the specific groups. The estimated ages of the TWA (TW Hya), 118TAU (118 Tau), US (Upper Scorpius), UCL (Upper Centaurus Lupus), and LCC (Lower Centaurus Crux) groups are from Gagné et al. (2018). For the BPMG (β Pic moving group), THA (Tucana-Horologium association), CAR (Carina), and COL (Columba) moving groups, the ages are from the recent work of Gratton et al. (2024). For HD 32297 and HD 141569 we have used their individual age estimates from Kalas (2005) and Wichittanakom et al. (2020), respectively. In the case of RZPsc, the quoted age combines the results of Punzi et al. (2018) and Potravnov et al. (2019). The 12CO line luminosities (L12CO) given in the 12th column refer to the J=2–1 rotational transition, except for NO Lup where the 3–2 line luminosity is quoted. The last column shows which label we use to mark the given object in Figs. 79. References to the stellar and disk parameters presented are summarized in the 14th column of the table.

References. 1. Ballering et al. (2013) - 2. Cataldi et al. (2023) - 3. Chen et al. (2014) - 4. Dent et al. (2014) - 5. Di Folco et al. (2020) - 6. Hales et al. (2022) - 7. Hardy et al. (2015) - 8. Hom et al. (2020) - 9. Kennedy et al. (2018) - 10. Kral et al. (2020b) - 11. Lacour et al. (2021) - 12. Lieman-Sifry et al. (2016) - 13. Lisse et al. (2017) - 14. Lovell et al. (2021b) - 15. Lovell et al. (2021a) - 16. MacGregor et al. (2018) - 17. MacGregor et al. (2019) - 18. Marino et al. (2016) - 19. Marino et al. (2020a) - 20. Marshall et al. (2021) - 21. Matrà et al. (2017a) - 22. Matrà et al. (2025) - 23. Meeus et al. (2012) - 24. Moór et al. (2011b) - 25. Moór et al. (2011a) - 26. Moór et al. (2015b) - 27. Moór et al. (2015a) - 28. Moór et al. (2016) - 29. Moór et al. (2017) - 30. Moór et al. (2019) - 31. Moór et al. (2020) - 32. Moór et al. (2021) - 33. Olofsson et al. (2013) - 34. Paegert et al. (2021) - 35. Pawellek et al. (2021) - 36. Pearce et al. (2022) - 37. Rebollido et al. (2022) - 38. Rhee et al. (2007) - 39. Riviere-Marichalar et al. (2014) - 40. Rodet et al. (2017) - 41. Schneiderman et al. (2021) - 42. Su et al. (2020) - 43. Su et al. (2023) - 44. Vican et al. (2016) - 45. Wichittanakom et al. (2020) - 46. Xiaoming et al. (in prep.) - 47. Zwintz et al. (2019) - 48. This work.

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