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Table 1

Overview of the sample and relevant stellar properties.

Name RA (J2000) Dec (J2000) Type d T eff L References
(h m s) (°′′′) (pc) (K) (L⊙)
1 LkHα 330 03 45 48.28 + 32 24 11.9 TT 250 ± 50 5800 1, 2, a
2 V892 Tau 04 18 40.61 + 28 19 15.5 HAe 142 ± 14 11 220 3, b
3 RY Tau 04 21 57.41 + 28 26 35.5 TT/HAe 142 ± 14 6310 3, b
4 LkCa 15 04 39 17.79 + 22 21 03.4 TT 142 ± 14 4350 3, c
5 DR Tau 04 47 06.20 + 16 58 42.8 TT 142 ± 14 4060 3, c
6 GM Aur 04 55 10.98 + 30 21 59.5 TT 142 ± 14 4730 3, c
7 AB Aur 04 55 45.84 + 30 33 04.2 HAe 139 ± 19 9800 4, d
8 SU Aur 04 55 59.38 + 30 34 01.5 TT/HAe 146 ± 50 5860 4, c
9 HD 31648 04 58 46.26 + 29 50 36.9 HAe 137 ± 25 8200 4, e
10 UX Ori 05 04 29.98 −03 47 14.2 HAe 460 ± 50 8710 5, 6, f
11 HD 36112 05 30 27.52 + 25 19 57.0 HAe 279 ± 70 7800 4, e
12 HD 36917 05 34 46.98 −05 34 14.5 HAe 375 ± 30 10 000 7, e
13 CQ Tau 05 35 58.46 + 24 44 54.0 HAe 113 ± 23 6750 4, b
14 V1247 Ori 05 38 05.24 −01 15 21.6 HAe 385 ± 15 7250 8, f
15 HD 38120 05 43 11.89 −04 59 49.8 HAe 375 ± 30 11 000 7, e
16 β Pic 05 47 17.08 −51 03 59.4 DD 19.44 ± 0.05 8052 4, g
17 HD 45677 06 28 17.42 −13 03 11.1 HBe 279 ± 73 21 380 4, h
18 VY Mon 06 31 06.92 + 10 26 04.9 embHAe 800 ± 300 12 023 9, 10, i
19 HD 259431 06 33 05.19 + 10 19 19.9 HAe 660 ± 100 14 000 7, e
20 R Mon 06 39 09.94 + 08 44 09.7 HBe 760 ± 300 30 903 10, j
21 HD 50138 06 51 33.39 −06 57 59.4 HBe 392 ± 86 15 490 4, h
22 HD 72106 08 29 34.89 −38 36 21.1 HAe 279 ± 88 8750 4, k
23 HD 87643 10 04 30.28 −58 39 52.0 HBe 1500 ± 500 17 000 11, l
24 CR Cha 10 59 06.97 −77 01 40.3 TT 160 ± 15 4900 12, m
25 HD 95881 11 01 57.61 −71 30 48.3 HAe 170 ± 30 8990 13, n
26 DI Cha 11 07 20.72 −77 38 07.2 TT 160 ± 15 5860 12, m
27 HD 97048 11 08 03.32 −77 39 17.4 HAe 158 ± 16 10 000 4, h
28 HP Cha 11 08 15.09 −77 33 53.1 TT 160 ± 15 4205 12, m
29 FM Cha 11 09 53.40 −76 34 25.5 TT 160 ± 15 4350 12, m
30 WW Cha 11 10 00.10 −76 34 57.8 TT 160 ± 15 4350 12, m
31 CV Cha 11 12 27.70 −76 44 22.3 TT 160 ± 15 5410 12, m
32 HD 98922 11 22 31.67 −53 22 11.4 HAe 1150 ± 515 10 500 4, e
33 HD 100453 11 33 05.57 −54 19 28.5 HAe 122 ± 10 7400 4, n
34 HD 100546 11 33 25.44 −70 11 41.2 HAe 97 ± 4 10 500 4, n
35 T Cha 11 57 13.55 −79 21 31.5 TT 108 ± 9 5890 14, h
36 HD 104237 12 00 05.08 −78 11 34.5 HAe 115 ± 5 8410 4, n
37 HD 109085 12 32 04.22 −16 11 45.6 DD 18.28 ± 0.06 6784 4, g
38 DK Cha 12 53 17.23 −77 07 10.7 embHAe 178 ± 18 7200 12, o
39 HD 135344 B 15 15 48.43 −37 09 16.0 HAe 142 ± 27 6750 15, e
40 HD 139614 15 40 46.38 −42 29 53.5 HAe 142 ± 27 7600 15, d
41 HD 142666 15 56 40.02 −22 01 40.0 HAe 140 ± 20 7900 7, 16, e
42 HD 142527 15 56 41.88 −42 19 23.2 HAe 233 ± 53 6260 4, n
43 HD 142560 15 56 42.31 −37 49 15.5 TT 150 ± 30 4000 17†, p
44 HD 143006 15 58 36.91 −22 57 15.2 TT 145 ± 15 5884 18, 19, 20, q
45 HD 144432 16 06 57.95 −27 43 09.7 HAe 160 ± 29 7500 4, e
46 HD 144668 16 08 34.28 −39 06 18.3 HAe 142 ± 27 8200 15, e
47 V2246 Oph 16 26 03.02 −24 23 36.0 TT 120 ± 5 5248 21, r
48 HBC 639 16 26 23.35 −24 20 59.7 TT 120 ± 5 5250 21, s
49 Elias 2-24 16 26 24.07 −24 16 13.5 TT 120 ± 5 4266 21, t
50 Elias 2-28 16 26 58.44 −24 45 31.8 TT 120 ± 5 4169 21, t
51 Elias 2-30 16 27 10.27 −24 19 12.7 TT/HAe 120 ± 5 5950 21, s
52 V2129 Oph 16 27 40.27 −24 22 04.1 TT 120 ± 5 3981 21, t
53 V2062 Oph 16 31 33.46 −24 27 37.2 TT 120 ± 5 4900 21, u
54 HD 150193 16 40 17.92 −23 53 45.1 HAe 216 ± 68 9500 4, e
55 AK Sco 16 54 44.84 −36 53 18.5 HAe 103 ± 21 6500 4, v
56 KK Oph 17 10 08.13 −27 15 18.8 HAe 160 ± 30 8030 5, 22, n
57 51 Oph 17 31 24.95 −23 57 45.5 HAe 124 ± 4 10 000 4, h
58 HD 163296 17 56 21.28 −21 57 21.8 HAe 119 ± 11 9200 4, d
59 HD 169142 18 24 29.77 −29 46 49.3 HAe 145 ± 15 7500 20, d
60 MWC 297 18 27 39.52 −03 49 52.0 HBe 250 ± 50 25 400 23†,w
61 MWC 300 18 29 25.69 −06 04 37.2 HBe 1800 ± 200 19 000 24, x
62 R CrA 19 01 53.65 −36 57 07.8 HAe 130 ± 20 11 100 25, 26, y
63 T CrA 19 01 58.77 −36 57 49.9 HAe 130 ± 20 6900 25, 26, y
64 HD 179218 19 11 11.25 + 15 47 15.6 HAe 254 ± 38 9640 4, d

Notes. HAe/HBe = Herbig Ae/Be star, TT = T Tauri star, embHAe = embedded Herbig Ae star, DD = debris disk object.

Reference. Distance references (†= 20-% error assumed): (1) Brown et al. (2008); (2) Kirk et al. (2006); (3) Wichmann et al. (1998); (4) van Leeuwen (2007); (5) Hillenbrand et al. (1992); (6) Bally et al. (2000); (7) Alecian et al. (2013); (8) Kraus et al. (2013); (9) Damiani et al. (1994); (10) Close et al. (1997); (11) Millour et al. (2009); (12) Whittet et al. (1997); (13) Verhoeff et al. (2010); (14) Torres et al. (2008); (15) Müller et al. (2011); (16) Preibisch & Mamajek (2008); (17) Comerón (2008); (18) de Zeeuw et al. (1999); (19) Bouwman et al. (2008); (20) Honda et al. (2012); (21) Loinard et al. (2008); (22) Leinert et al. (2004); (23) Drew et al. (1997); (24) Miroshnichenko et al. (2004); (25) Marraco & Rydgren (1981); (26) Prato et al. (2003). Effective-temperature references: (a) Brown et al. (2008); (b) Hernández et al. (2004); (c) Kenyon & Hartmann (1995); (d) Folsom et al. (2012); (e) Alecian et al. (2013); (f) Mora et al. (2002); (g) Gray et al. (2006); (h) van den Ancker et al. (1998); (i) Testi et al. (1998); (j) Hillenbrand et al. (1992); (k) Folsom et al. (2008); (l) Kraus (2009); (m) Luhman (2007); (n) Acke et al. (2010); (o) Spezzi et al. (2008); (p) Stempels et al. (2007); (q) Bouwman et al. (2008); (r) Massarotti et al. (2005); (s) Prato et al. (2003); (t) Natta et al. (2006); (u) Kim et al. (2013); (v) Alencar et al. (2003); (w) Acke et al. (2008); (x) Miroshnichenko et al. (2004); (y) Bibo et al. (1992).

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