Table A.1

Most reliable parameters obtained with the 8 data sets.

ΦM ΦD a θ
[mas] [mas] [mas] [deg]
Period A1: mjd ~  54781 and 54783 (AMBER data)

Free ? Yes Yes Yes Yes
Value 2.24 12.35 4.2 135 0.71
Error (1-σ) 2.7 × 10-2 2.3 × 10-1 3.5 × 10-2 0.35
Period A2: mjd ~  54826 (AMBER data)

Free ? Yes No Yes Yes
Value 2.05 12.2 3.8 69 0.20
Error (1-σ) 2.9 × 10-2 4.9 × 10-2 0.53
Period A3: mjd ~  54883 and 54890 (AMBER data)

Free ? Yes Yes Yes Yes
Value 2.14 12.2 4.5 347 1.36
Error (1-σ) 4.3 × 10-2 2.3 × 10-1 3.8 × 10-2 0.37
Period A4: mjd ~  54928 (AMBER data)

Free ? Yes No Yes Yes
Value 1.98 12.2 4.2 291 1.62
Error (1-σ) 3.9 × 10-2 4.0 × 10-2 0.47
Period P1: mjd ~  55500 (PIONIER data)

Free ? Yes No Yes Yes
Value 2.17 12.2 3.9 32 1.58
Error (1-σ) 1.4 × 10-2 1.5 × 10-2 0.06
Period P2: mjd ~  55529 (PIONIER data)

Free ? Yes No Yes Yes
Value 2.27 12.2 4.5 351 2.46
Error (1-σ) 1.2 × 10-2 0.2 × 10-2 0.78
Period P3: mjd ~  55537 (PIONIER data)

Free ? Yes No Yes Yes
Value 2.19 12.2 4.5 346 0.96
Error (1-σ) 1.6 × 10-2 0.6 × 10-2 0.20
Period P4: mjd ~  55552 (PIONIER data)

Free ? Yes No Yes Yes
Value 2.30 12.2 4.42 330.6 0.96
Error (1-σ) 0.9 × 10-2 0.9 × 10-2 0.12

Notes. The errors are the result of Monte Carlo computations based on the error on the visbilities and closure phases measurements.φM and φD are the M star diameter and the dusty disc/envelope FWHM, respectively. a and θ are the visual separation and orientation of the binary. The last column gives the final reduced χ2 of the fit.

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