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Table 2.
Journal of ESPaDOnS observations of DoAr 44.
| Date | UT | HJD | Φrot | S/N |
|---|---|---|---|---|
| (2019) | (hh:mm:ss) | (2 450 000.+) | (731 nm) | |
| Mar 15 | 14:31:32 | 8558.10852 | 0.48 | 137 |
| Mar 16 | 15:32:19 | 8559.15082 | 0.83 | 141 |
| Mar 18 | 15:11:40 | 8561.13665 | 1.50 | 133 |
| Mar 19 | 14:47:48 | 8562.12015 | 1.83 | 124 |
| Mar 20 | 14:13:53 | 8563.09667 | 2.16 | 131 |
| Mar 21 | 14:50:36 | 8564.12225 | 2.51 | 132 |
| Mar 22 | 13:32:39 | 8565.06818 | 2.83 | 143 |
| Jun 08 | 09:16:27 | 8642.89230 | 29.12 | 139 |
| Jun 09 | 09:21:13 | 8643.89558 | 29.46 | 135 |
| Jun 10 | 09:19:12 | 8644.89415 | 29.80 | 135 |
| Jun 11 | 10:15:19 | 8645.93308 | 30.15 | 134 |
| Jun 12 | 10:07:45 | 8646.92779 | 30.48 | 130 |
Notes. All observations consist of sequences of four subexposures, each lasting 950 s. Columns respectively list, for each observation, the UT date, time, heliocentric Julian date (HJD), rotational phase, and signal-to-noise ratio (S/N) at 731 nm (per 2.6 km s−1 velocity bin).
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