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Table A.1.
Dates of the observations of W Hya, R Dor, and IK Tau in which we detected OH lines or obtained a meaningful upper limit (UL).
| Star | Band | Proj. code | Lines (v, NJ) | Date | Φ |
|---|---|---|---|---|---|
| W Hya | 4 | 2017.1.00075.S | 0, 1325/2; 1, 1021/2 | 17-10-18 | 1.0 |
| 6 | 2016.1.00374.S | 0, 1835/2 | 17-07-08 | 0.7 | |
| 7 | 2016.A.00029.S | 1, 1735/2 | 17-11-25 | 1.1 | |
| R Dor | 3 | 2017.1.00582.S | 0, 1223/2 | 17-12-18 | 0.7 |
| 4 | 2016.1.00004.S | 0, 1325/2 (UL) | 17-09-26 | 0.5 | |
| 6 | 2017.1.00582.S | 0, 1429/2 | 18-01-05 | 0.75 | |
| 7 | 2017.1.00582.S | 0, 1633/2 | 18-01-06 | 0.75 | |
| 7 | 2015.1.00166.S | 0, 1735/2 | 15-08-31 | −1.5 | |
| IK Tau | 6 | 2017.1.00582.S | 0, 1429/2 | 18-01-04 | 0.1 |
Notes. We also give the approximate stellar pulsation phase when the observations were acquired (Φ). Negative values denote observations obtained at earlier epochs than the ones we obtained.
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