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Table 3

Detections (marked in gray) and non-detections of extended emission and closure-phase signal.

HD fCSE [%] σf [%] χ f V 2 Comp. HD fCSE [%] σf [%] χ f V 2 Comp.
142 –0.69 0.26 –2.61 1.05 no no 91324 0.14 0.17 0.82 0.38 no no
1581 –0.21 0.31 –0.67 1.00 no no 99211 0.35 0.22 1.60 0.75 no no
2262 0.67 0.18 3.72 0.51 yes no 102365 0.43 0.23 1.91 0.66 no no
3302 0.36 0.26 1.36 1.22 no no 104731 0.52 0.14 3.73 0.55 yes no
3823 0.25 0.22 1.16 0.78 no no 108767 0.57 0.15 3.73 0.54 yes no
4150 2.57 0.49 5.22 2.83 yes yes 109787 –0.32 0.20 –1.61 0.73 no no
7570 –0.36 0.26 –1.36 1.17 no no 115617 0.09 0.23 0.40 0.40 no no
7788 1.43 0.17 8.53 0.47 yes no 120136 –0.21 0.22 –0.96 0.65 no no
10647 –0.08 0.26 –0.31 0.81 no no 128898 0.15 0.22 0.69 0.75 no no
11171 –0.06 0.42 –0.14 1.30 no no 129502 –0.04 0.14 –0.29 0.38 no no
14412 0.96 0.21 4.66 0.74 yes no 130109 –0.41 0.43 –0.96 1.75 no no
15008 0.56 0.32 1.73 1.22 no no 134083 –0.56 0.47 –1.18 2.64 no no
15798 3.03 0.34 8.82 0.68 yes no1 135379 0.18 0.37 0.48 1.01 no no
16555 40.55 2.45 16.55 ... yes yes 136202 –1.56 0.64 –2.46 3.03 no no
17051 –0.24 0.23 –1.06 0.96 no no 139664 0.11 0.19 0.59 0.62 no no
17925 –0.05 0.23 –0.22 0.70 no no 141891 –0.1 0.20 –0.50 0.64 no no
19107 0.47 0.21 2.28 0.49 no no 149661 0.14 0.22 0.65 1.70 no no
20766 0.08 0.26 0.30 1.18 no no 152391 0.06 0.18 0.34 0.58 no no
20794 1.64 0.37 4.46 1.58 yes no 160032 0.01 0.11 0.09 0.28 no no
20807 –0.05 0.53 –0.09 3.74 no no 160915 0.19 0.28 0.67 0.67 no no
22001 0.3 0.20 1.53 0.71 no no 164259 –0.18 0.19 –0.96 0.62 no no
23249 2.44 0.37 6.65 2.17 yes no 165777 0.46 0.28 1.62 0.98 no no
25457 –0.07 0.14 –0.50 0.37 no no 172555 0.55 0.25 2.16 1.09 no no
28355 0.88 0.09 9.33 0.36 yes no 178253 0.15 0.36 0.41 1.68 no no
29388 3.84 0.46 8.35 3.02 yes yes 182572 0.09 0.13 0.69 0.37 no no
30495 –0.14 0.21 –0.68 0.46 no no 188228 0.53 0.27 1.99 0.82 no no
31295 0.21 0.15 1.41 0.54 no no 192425 –0.31 0.25 –1.26 1.03 no no
31925 0.41 0.22 1.90 0.63 no no 195627 0.05 0.52 0.10 2.87 no no
33111 0 0.41 0.00 2.00 no no 197157 0.35 0.30 1.15 1.03 no no
33262 0.27 0.21 1.31 0.58 no no 197692 –0.14 0.20 –0.71 0.48 no no
34721 –0.36 0.21 –1.75 0.61 no no 202730 29.56 9.96 2.97 ... no yes
38858 –0.69 0.29 –2.34 1.10 no no 203608 –0.74 0.34 –2.15 1.52 no no
39060 0.88 0.23 3.90 0.49 yes no 206860 0.21 0.30 0.69 1.24 no no
40307 –0.34 0.24 –1.44 1.06 no no 207129 0.13 0.13 1.00 0.26 no no
43162 0.4 0.21 1.94 0.63 no no 210049 0.18 0.38 0.47 2.67 no no
45184 0.42 0.15 2.83 0.53 no no 210277 –0.41 0.31 –1.31 1.85 no no
53705 0.08 0.23 0.35 0.67 no no 210302 0.83 0.25 3.39 1.07 yes no
56537 –0.42 0.25 –1.68 0.98 no no 210418 –0.43 0.29 –1.46 1.17 no no
69830 0.04 0.26 0.15 1.01 no no 213845 –0.43 0.24 –1.81 0.82 no no
71155 0.09 0.25 0.35 1.16 no no 214953 –0.15 0.22 –0.69 0.71 no no
72673 0 0.33 0.00 1.89 no no 215648 –0.21 0.22 –0.96 0.76 no no
76151 0.16 0.28 0.56 1.38 no no 215789 –0.2 0.26 –0.78 0.68 no no
76932 –0.04 0.42 –0.09 2.79 no no 216435 –0.35 0.27 –1.27 1.14 no no
82434 0.39 0.58 0.68 3.72 no no 219482 0.2 0.17 1.19 0.53 no no
88955 –0.25 0.25 –1.02 1.00 no no 219571 0.09 0.27 0.33 0.78 no no
90132 –0.74 0.41 –1.79 1.80 no no 224392 1.74 0.27 6.34 1.15 yes yes

Notes. Detections, i.e., stars with significant excess but without a companion following Marion et al. (2014), are marked in gray. The quantity fCSE is the disk-to-star flux ratio. The quantity σf is the 1σ uncertainty on that measurement, χf = fCSE/σf gives the significance of the detection, and gives the reduced χ2 of the fit of our model to the data. The columns named “V2” and “Comp.” include notes on whether there is a significant detection of extended emission or of closure-phase signal, respectively.

(1)

See notes in Sect. 4.1.

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