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Table 1
VLTI/AMBER observations.
| Target | Date | Mode | Baselines | PA |
| (Sp. type) | K- | BL1/BL2/BL3 | ||
| μm | m | deg | ||
|
|
||||
| AH Sco | 2010-06-04 | 2.1 | 40.6/40.4/62.3 | 168/–51/–91 |
| (M4-5) | 2010-06-04 | 2.3 | 40.8/45.2/66.7 | 159/–63/–99 |
| UY Sct | 2010-06-04 | 2.1 | 37.6/43.4/58.5 | 163/–64/–103 |
| (M4) | 2010-06-04 | 2.3 | 36.9/37.4/49.8 | 172/–56/–102 |
| KW Sgr | 2012-04-21 | 2.1 | 62.9/71.5/70.1 | 64/–178/129 |
| (M1.5) | 2012-04-21 | 2.3 | 63.7/71.4/71.5 | 73/–170/137 |
Notes.The AMBER instrument mode is K-2.1 μm (medium-resolution mode with range 1.92–2.26 μm) or K-2.3 μm (2.12–2.47 μm). The baseline is the projected baseline length for the AT VLTI baseline used.
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