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Table 1

Log of the series of AMBER observations.

Object Seeing Coherence time DIT1 Telescopes Baselines PAs
(′′) (ms) (ms) (m) (°)

2012/04/06
HD 84177 0.81 2.98 500.0 UT1-UT2-UT3 50.0/43.3/92.6 23.8/37.7/30.3
HD 85567 0.78 3.10 500.0 UT1-UT2-UT3 48.4/42.1/89.8 28.5/43.1/35.2
HD 85313 0.78 3.11 500.0 UT1-UT2-UT3 48.0/41.5/88.7 32.1/47.3/39.1
2012/05/06
HD 84177 0.88 5.60 500.0 UT2-UT3-UT4 41.8/89.0/61.3 226.7/84.2/108.8
HD 85567 1.06 4.95 500.0 UT2-UT3-UT4 40.5/88.3/61.8 231.7/89.8/113.6
HD 85313 0.55 8.52 500.0 UT2-UT3-UT4 37.6/85.5/62.5 242.9/104.4/127.9
2012/12/29
HD 84177 0.55 4.11 500.0 UT2-UT3-UT4 44.5/88.4/56.1 205.7/58.2/83.4
HD 85567 0.52 4.35 500.0 UT2-UT3-UT4 44.0/88.9/56.9 208.2/60.7/85.3
HD 85313 0.70 3.31 500.0 UT2-UT3-UT4 43.8/89.2/58.0 211.9/65.6/90.3
2013/03/04
HD 84177 0.86 4.33 500. 0 UT1-UT2-UT3 50.0/43.3/92.6 23.7/37.6/30.1
HD 85567 0.55 5.80 500.0 UT1-UT2-UT3 48.9/42.6/90.8 25.8/40.0/32.4
HD 85313 0.54 6.64 500. 0 UT1-UT2-UT3 48.7/42.2/90.1 28.9/43.6/35.7

Notes.

(1)

DIT represents the detector integration time.

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