Table A.1
Observing log of our Stokes VQU spectropolarimetric SPIRou observations of AU Mic in August 2023
| BJD | UT date | Star | c/ϕ | texp | S/N | σP | Stokes | Bℓ | <Bs> | dT |
|---|---|---|---|---|---|---|---|---|---|---|
| (2459000+) | (s) | (H) | (10−4 Ic) | (G) | (kG) | (K) | ||||
| 1158.9450165 | 02 Aug 2023 | AU Mic | 238/0.466 | 802.4 | 834 | 0.81 | V | 5±4 | 2.51±0.05 | 19.19±1.18 |
| 1158.9557904 | 02 Aug 2023 | AU Mic | 238/0.468 | 802.4 | 845 | 0.63 | Q | |||
| 1158.9664817 | 02 Aug 2023 | AU Mic | 238/0.470 | 802.4 | 845 | 0.64 | U | |||
| 1159.8927438 | 03 Aug 2023 | AU Mic | 238 0.661 | 802.4 | 889 | 0.80 | V | 93±4 | 2.62±0.05 | 3.70±1.14 |
| 1159.9035273 | 03 Aug 2023 | AU Mic | 238 0.663 | 802.4 | 876 | 0.61 | Q | |||
| 1159.9143589 | 03 Aug 2023 | AU Mic | 238 0.666 | 802.4 | 895 | 0.61 | U | |||
| 1160.9676210 | 04 Aug 2023 | AU Mic | 238 0.882 | 802.4 | 920 | 0.74 | V | −13±4 | 2.54±0.04 | 16.45±1.31 |
| 1161.9622558 | 05 Aug 2023 | AU Mic | 239 0.087 | 802.4 | 893 | 0.95 | V | 76±5 | 2.81±0.03 | -6.09±1.21 |
| 1165.8684823 | 09 Aug 2023 | AU Mic | 239 0.891 | 802.4 | 908 | 0.80 | V | −12±4 | 2.57±0.04 | 13.82±1.26 |
| 1165.8795421 | 09 Aug 2023 | AU Mic | 239 0.893 | 802.4 | 925 | 0.64 | Q | |||
| 1165.8903909 | 09 Aug 2023 | AU Mic | 239 0.895 | 802.4 | 923 | 0.61 | U | |||
| 1166.8725352 | 10 Aug 2023 | AU Mic | 240 0.097 | 802.4 | 882 | 0.77 | V | 62±4 | 2.80±0.03 | -6.97±1.21 |
| 1166.8834741 | 10 Aug 2023 | AU Mic | 240 0.099 | 802.4 | 850 | 0.59 | Q | |||
| 1166.8938495 | 10 Aug 2023 | AU Mic | 240 0.102 | 802.4 | 772 | 0.65 | U | |||
| 1167.8481084 | 11 Aug 2023 | AU Mic | 240 0.298 | 802.4 | 904 | 0.84 | V | 11±4 | 2.79±0.04 | 1.06±1.25 |
| 1167.8590500 | 11 Aug 2023 | AU Mic | 240 0.300 | 802.4 | 907 | 0.63 | Q | |||
| 1167.8697311 | 11 Aug 2023 | AU Mic | 240 0.302 | 802.4 | 905 | 0.64 | U | |||
| 1179.8186449 | 23 Aug 2023 | AU Mic | 242 0.761 | 802.4 | 844 | 0.86 | V | 79±4 | 2.44±0.05 | 12.64±1.16 |
| 1179.8302123 | 23 Aug 2023 | AU Mic | 242 0.763 | 802.4 | 860 | 0.63 | Q | |||
| 1179.8420478 | 23 Aug 2023 | AU Mic | 242 0.766 | 802.4 | 880 | 0.66 | U | |||
| 1180.9308369 | 24 Aug 2023 | AU Mic | 242 0.990 | 802.4 | 867 | 0.92 | V | 17±4 | 2.61±0.04 | 5.83±1.13 |
| 1181.8186111 | 25 Aug 2023 | AU Mic | 243 0.173 | 802.4 | 866 | 0.84 | V | -16±4 | 2.88±0.03 | -9.74±1.31 |
| 1181.8298154 | 25 Aug 2023 | AU Mic | 243 0.175 | 802.4 | 851 | 0.63 | Q | |||
| 1181.8406102 | 25 Aug 2023 | AU Mic | 243 0.177 | 802.4 | 837 | 0.65 | U | |||
| 1182.8234064 | 26 Aug 2023 | AU Mic | 243 0.379 | 802.4 | 830 | 0.94 | V | 27±5 | 2.50±0.05 | 15.01 ±1.31 |
| 1182.8342156 | 26 Aug 2023 | AU Mic | 243 0.382 | 802.4 | 832 | 0.66 | Q | |||
| 1182.8451345 | 26 Aug 2023 | AU Mic | 243 0.384 | 802.4 | 831 | 0.66 | U | |||
| 1184.8133935 | 28 Aug 2023 | AU Mic | 243 0.789 | 802.4 | 894 | 0.90 | V | 71±4 | 2.40±0.06 | |
| 1185.7993039 | 29 Aug 2023 | AU Mic | 243 0.992 | 802.4 | 902 | 0.82 | V | 14±4 | 2.57±0.04 | 6.39±1.23 |
| 1185.8100395 | 29 Aug 2023 | AU Mic | 243 0.994 | 802.4 | 908 | 0.58 | Q | |||
| 1185.8207370 | 29 Aug 2023 | AU Mic | 243 0.996 | 802.4 | 891 | 0.73 | U | |||
| 1186.8327092 | 30 Aug 2023 | AU Mic | 244 0.204 | 802.4 | 740 | 0.91 | V | −20±4 | 2.83±0.03 | -10.81±1.19 |
| 1186.8438843 | 30 Aug 2023 | AU Mic | 244 0.207 | 802.4 | 717 | 0.70 | Q | |||
| 1186.8546516 | 30 Aug 2023 | AU Mic | 244 0.209 | 802.4 | 709 | 0.71 | U | |||
| 1187.7936592 | 31 Aug 2023 | AU Mic | 244 0.402 | 802.4 | 670 | 0.95 | V | 16±5 | 18.52±1.16 | |
| 1187.8247707 | 31 Aug 2023 | AU Mic | 244 0.408 | 802.4 | 691 | 0.71 | Q | |||
| 1187.8355074 | 31 Aug 2023 | AU Mic | 244 0.411 | 802.4 | 650 | 0.74 | U | |||
| 1188.7797490 | 01 Sep 2023 | AU Mic | 244 0.605 | 802.4 | 870 | 0.77 | V | 92±4 | 2.54±0.04 | 11.29±1.07 |
| 1188.7903324 | 01 Sep 2023 | AU Mic | 244 0.607 | 802.4 | 882 | 0.64 | Q | |||
| 1188.8013085 | 01 Sep 2023 | AU Mic | 244 0.609 | 802.4 | 896 | 0.61 | U |
Notes. All exposures consist of 4 sub-exposures of equal length. For each star and each visit, we list the barycentric Julian date BJD, the UT date, the rotation cycle c and phase ϕ (computed as indicated in Sect. 3), the total observing time texp, the peak S/N in the spectrum (in the H band) per 2.3 km s−1 pixel, the noise level in the LSD Stokes profile, the estimated Bℓ with error bars (for Stokes V profiles only), the measured small-scale field <Bs> and differential temperature dT with error bars (for each observing night).
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