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Table 1

Position, spectral type, distance, H magnitude, and binarity of the sample.

Star RA Dec SpT Dist.(pc) Log(L/L) Refs. H-mag Resolved? Binary?

V380 Ori 05 36 25 –06 42 57 A1e 510 1.99 1, 2, 3 6.96 yes Unresolved, Border
TWA 07 10 42 30 –33 40 16 M3.2 34 –0.94 4 7.13 no no
TW Hya 11 01 51 –34 42 17 M0.5 56 –0.72 4 7.55 marginally no
WW Cha 11 10 00 –76 34 57 K5 160 0.74 5, 6 7.21 yes Yes
TWA 3A 11 10 28 –37 31 52 M4.1 35 –0.92 4 7.53 yes Yes, Outside
TWA 3B 11 10 28 –37 31 52 M4.0 35 –1.10 4 8.15 no Outside
HT Lup 15 45 12 –34 17 30 K2 150 0.74 4 6.87 yes Border, Outside
HN Lup 15 48 05 –35 15 52 M1.5 150 –0.28 7, 14 8.1 yes Outside
GQ Lup 15 49 12 –35 39 05 K7 150 0.17 27 7.70 yes Outside
RU Lup 15 56 42 –37 49 15 K7 150 0.16 8, 9, 22 7.82 yes no
V1149 Sco 15 58 36 –22 57 15 G6 145 0.39 10 7.69 yes no
RY Lup 15 59 28 –40 21 51 G0V 150 0.41 2, 11, 12 7.69 yes no
MY Lup 16 00 44 –41 55 31 K0 150 –0.20 13, 23 8.69 no no
V1000 Sco 16 11 08 –19 04 46 K2 145 0.44 14, 24 7.98 yes Yes
AS 205 A 16 11 31 –18 38 24 K5 125 0.60 15 6.75 yes Outside
V2129 Oph 16 27 40 –24 22 04 K5 121 0.15 26 7.67 yes no
V2508 Oph 16 48 45 –14 16 35 K6 125 0.46 16, 17 7.57 yes no
V1121 Oph 16 49 15 –14 22 08 K5 130 0.176 2, 12 7.45 yes no
AK Sco 16 54 44 –36 53 18 F5V 145 0.61 × 2 18, 22 7.06 yes Yes
V4046 Sgr 18 14 10 –32 47 34 K5V 73 –0.41 × 2 19 7.44 no Unresolved
FK Ser 18 20 22 –10 11 13 K6IV 32 0.2 2, 20, 25 6.92 no Outside
S CrA N 19 01 08 –36 57 19 K3 130 0.36 15 7.05 yes Outside
V709 CrA 19 01 34 –37 00 56 K1IV 130 0.19 21 7.97 no no

Notes. For the binarity, “Unresolved” means that the companion is unresolved by PIONIER, “Yes” means that the star has a detected companion in PIONIER’s half field of view (125 mas), “Border” that the companion lies on the edge of the field of view, stars with “Outside” have a companion with a separation much larger than the field of view, and “no” indicates that the star is single.

Reference. (1) Manoj et al. (2006); (2) van Leeuwen (2007); (3) Alecian et al. (2013); (4) Herczeg & Hillenbrand (2014); (5) Luhman (2007); (6) Whittet et al. (1997); (7) Hughes et al. (1994); (8) Lommen et al. (2007); (9) Stempels et al. (2007); (10) Yang et al. (2012); (11) Reipurth et al. (1996); (12) Artemenko et al. (2012); (13) Romero et al. (2012); (14) Sartori et al. (2003); (15) Bast et al. (2011); (16) Andrews et al. (2010); (17) de Geus et al. (1989); (18) Alencar et al. (2003); (19) Donati et al. (2011); (20) Torres et al. (2006); (21) Forbrich & Preibisch (2007); (22) this paper; (23) Gregorio-Hetem & Hetem (2002); (24) Wahhaj et al. (2010); (25) McDonald et al. (2012); (26) Donati et al. (2011); (27) Dai et al. (2010).

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