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Table 1

Log of the observations.

Date UT HA Baselines λ 0 V 2 σ stat σ syst r 0
(h) (h) Telescopes Bp (m) PA (°) (nm) (cm)

28-08-2013 11.6 –1.8 S1S2 24 –172 712.5 1.026 0.094 0.001 8
28-08-2013 12.2 –1.1 S1S2 23 180 712.5 0.988 0.092 0.001 9
S1E2 221 –149 712.5 0.610 0.092 0.016

29-08-2013 10.7 –2.6 S1S2 25 –164 712.5 0.998 0.125 0.001 8
29-08-2013 11.9 –1.3 S1S2 23 –178 712.5 1.036 0.125 0.001 10
S2E2 205 –145 712.5 0.618 0.055 0.012
S1E2 225 –148 712.5 0.628 0.074 0.015
12.2 –1.1 S1S2 23 179 712.5 1.025 0.091 0.001 10
S2E2 200 –146 712.5 0.543 0.050 0.011
12.8 –0.47 S1S2 24 172 712.5 0.965 0.073 0.001 9
S2E2 187 –150 712.5 0.635 0.049 0.013

02-11-2013 8.2 –0.8 W1W2 100 89 730 0.859 0.030 0.004 7
9.1 0.1 W1W2 106 92 730 0.837 0.037 0.004 7

27-08-2014 11.8 –1.5 E2W2 156 –112 552.5 0.505 0.018 0.008 9
E1W2 222 –113 552.5 0.510 0.034 0.015
E2W2 155 –110 707.5 0.781 0.030 0.007
27-08-2014 12.5 –0.88 E1W2 217 –114 552.5 0.404 0.042 0.013 9
E1E2 64 –113 707.5 0.970 0.068 0.002
E2W2 155 –110 707.5 0.711 0.038 0.007

Notes. Columns 13 give the date, the UT time, and the hour angle (HA) of the observations. Columns 46 give the telescope pair, the projected baseline length Bp, and its orientation PA. Column 7 gives the central wavelength of the spectral range used to compute the squared visibility. Columns 810 give the calibrated squared visibility V2, the statistic error on V2, and the systematic error on V2 (see text for details). Column 11 provides the Fried parameter at 550 nm for each observation.

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