Table 1
VLTI/AMBER observations.
| Target (Sp. type) | Date | Baseline | Projected baseline | PA | Calibrator | |||
| m | deg | |||||||
|
|
||||||||
| ϵ Oct (M5 III) | 2012 Jun. 25 | D0-A1-C1 | 28.9/15.4/15.1 | –119/79/–138 | HIP 104755 | |||
| 2012 Aug. 02 | B2-A1-C1 | 10.26/15.62/7.83 | –96.1/57.8/22.7 | HIP 104755 | ||||
| β Peg (M2.5 II-III) | 2012 Jun. 25 | D0-A1-C1 | 30.4/15.6/16.4 | –122/76.6/140 | HIP 114144 – HIP 1168 | |||
| 2012 Aug. 09 | B2-A1-C1 | 11.1/14.5/7.0 | –69.2/82.80/35.20 | HIP 114144 – HIP 1168 | ||||
| NU Pav (M6 III) | 2012 Aug. 02 | B2-A1-C1 | 10.9/15.8/9.8 | –70.6/71.6/28.8 | HIP 82363 | |||
| ψ Peg (M3 III) | 2012 Jun. 16 | D0-I1-G1 | 82.1/32.8/66.1 | 102/–128/124.5 | HIP 114144 – HIP 1168 | |||
| γ Hya (G8 III) | 2013 Mar. 16 | A1-G1-J3 | 74.9/132.2/135.7 | 118/15.3/47.7 | K Hya | |||
Notes. Details of our observations. The AMBER instrument mode is K-2.3 μm (2.12–2.47 μm). The projected baseline is the projected baseline length for the AT VLTI baseline used, and PA is the position angle of the baseline (north through east). γ Hya has been observed in K-2.1 and K-2.3 bands, which together cover the range 1.9–2.47 μm.
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