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Table A.1.

Technical overview of the PIONIER observations of PDS 27 and PDS 37 over two nights in March 2015.

Source MJD Baseline τcoh Seeing V2 Closure Phase
(m) (ms) (arcsec) (°)
PDS 27 57083.13889 44.0 6.7 0.83 0.35 ± 0.02
45.2 0.48 ± 0.02
55.3 0.50 ± 0.03
56.1 0.55 ± 0.02
98.7 0.19 ± 0.01 −2.4 ± 0.9
100.4 0.32 ± 0.02 −0.9 ± 1.8
57084.13284 45.3 5 0.93 0.27 ± 0.01
55.7 0.09 ± 0.01
56.1 0.48 ± 0.01
80.3 0.32 ± 0.02 0.7 ± 2.9
100.7 0.16 ± 0.01 −5.6 ± 2.1
121.4 0.22 ± 0.02 −4.4 ± 2.0/
4.7 ± 1.9

PDS 37 57084.18331 42.0 4.7 0.86 0.24 ± 0.01
43.3 0.58 ± 0.01
49.1 0.54 ± 0.01
50.4 0.70 ± 0.02
60.5 0.3 ± 0.01
61.8 0.09 ± 0.01
88.9 0.38 ± 0.02 0.2 ± 2.0
89.5 0.53 ± 0.01 0.4 ± 0.6
90.3 0.14 ± 0.01 −1.0 ± 2.5
93.0 0.56 ± 0.03 −1.0 ± 3
124.4 0.32 ± 0.01 4.0 ± 3.1/
−0.7 ± 2.8
127.4 0.45 ± 0.01 −0.3 ± 2.4/
1.5 ± 1.8

Notes. The closure phases are the product of three baselines, and we report them at the highest spatial frequency (longest baseline of the triplet).

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