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Table 3

Occultation model parameters found for the AA Tau-like candidates.

CSIMon ID Epoch Rw(R) h max / R w φw(°) Inclination (°)

CSIMon-000056 2008 9.29 0.24–0.25 (±0.10) 320 (±40)–360 71 ± 6
CSIMon-000056 2011 9.45 0.24–0.26 (±0.10) 290 (±70)–360 71 ± 6
CSIMon-000250 2008 11.71 0.23–0.28 (±0.05) 140 (±30)–360 74 ± 3
CSIMon-000250 2011 12.28 0.24–0.27 (±0.05) 270 (±30)–360 74 ± 3
CSIMon-000296 2011 6.86 0.21–0.31 (±0.09) 290 (±40)–360 72 ± 5
CSIMon-000297 2008 5.95 0.17–0.28 (±0.04) 180 (±30)–360 75 ± 2
CSIMon-000358 2011 6.51 0.17–0.19 (±0.06) 210 (±50)–360 73 ± 4
CSIMon-000379 2011 5.89 0.22–0.34 (±0.12) 110 (±30)–270 (±90) 70 ± 7
CSIMon-000441 2008 3.97 0.17–0.23 (±0.11) 160 (±20)–310 (±50) 70 ± 7
CSIMon-000456 2011 6.92 0.18–0.24 (±0.05) 360 74 ± 3
CSIMon-000498 2008 4.73 0.17–0.21 (±0.10) 145 (±35)–165 (±15) 70 ± 6
CSIMon-000498 2011 4.77 0.19–0.22 (±0.10) 130 (±50)–165 (±15) 70 ± 6
CSIMon-000654 2008 3.87 0.10–0.13 (±0.06) 180 (±60)–310 (±50) 73 ± 4
CSIMon-000660 2008 7.64 0.25–0.33 (±0.04) 260 (±20)–360 74 ± 3
CSIMon-000660 2011 7.50 0.27–0.29 (±0.05) 200 (±30)–360 74 ± 3
CSIMon-000774 2008 4.73 0.15–0.21 (±0.03) 220 (±40)–360 75 ± 2
CSIMon-000811 2011 8.19 0.26–0.28 (±0.08) 360 72 ± 5
CSIMon-000824 2008 7.90 0.24–0.27 (±0.08) 260 (±40)–360 72 ± 5
CSIMon-000928 2008 6.36 0.28–0.30 (±0.10) 120300 (±60) 71 ± 6
CSIMon-001054 2011 3.52 0.16–0.21 (±0.09) 270 (±70)–360 70 ± 5
CSIMon-001140 2008 6.79 0.16–0.24 (±0.03) 190 (±20)–360 75 ± 2
CSIMon-001140 2011 6.83 0.14–0.24 (±0.03) 190 (±20)–360 75 ± 2
CSIMon-001167 2011 5.37 0.15–0.18 (±0.05) 330 (±30)–360 74 ± 3
CSIMon-001296 2011 8.52 0.31–0.34 (±0.13) 260 (±80)–330 (±30) 69 ± 8
CSIMon-001308 2008 7.86 0.28–0.30 (±0.06) 330 (±30)–360 73 ± 4
CSIMon-001308 2011 8.04 0.20–0.27 (±0.06) 340 (±20)–360 73 ± 4
CSIMon-014132 2011 3.98 0.18–0.32 (±0.14) 120 (±40)–290 (±80) 68 ± 9

Notes. Rw is the radius where the warp is located, assumed to be at the co-rotation radius (i.e., Rw = Rco); hmax is the maximum warp height found for each flux dip, expressed in stellar radii R; and φw is the azimuthal extension of the warp found for each flux dip. The inclinations shown here were constrained using the occultation model.

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