Table A.1.
Observations for StKM 1-1262.
| Date | UT | HJD | ncyc | texp | S/N | σLSD | Bℓ | ⟨BI⟩ | Teff |
|---|---|---|---|---|---|---|---|---|---|
| [hh:mm:ss] | [−2460330.1563] | [s] | [10−5Ic] | [G] | [kG] | [K] | |||
| January 20 | 15:45:04.50 | 0.0000 | 0.00 | 4x523 | 254 | 8.7 | −80.0 ± 12.9 | 4.38 ± 0.07 | 3906 ± 4 |
| January 21 | 15:50:58.02 | 1.0041 | 0.81 | 4x523 | 271 | 7.2 | −56.8 ± 10.7 | 4.04 ± 0.08 | 3921 ± 4 |
| January 23 | 15:36:47.78 | 2.9943 | 2.41 | 4x523 | 244 | 9.3 | −44.8 ± 12.4 | 3.48 ± 0.07 | 3945 ± 3 |
| January 30 | 15:34:46.05 | 9.9928 | 8.06 | 4x523 | 271 | 7.4 | −127.0 ± 10.9 | 4.24 ± 0.06 | 3912 ± 3 |
| February 15 | 12:55:56.27 | 25.8825 | 20.87 | 4x523 | 254 | 7.6 | −7.9 ± 11.5 | 4.19 ± 0.07 | 3918 ± 3 |
| February 17 | 14:12:10.61 | 27.9355 | 22.53 | 4x523 | 229 | 9.7 | −98.9 ± 13.4 | 3.51 ± 0.07 | 3961 ± 3 |
| February 18 | 15:05:37.19 | 28.9726 | 23.37 | 4x523 | 216 | 11.3 | −13.3 ± 14.6 | 3.48 ± 0.07 | 3948 ± 4 |
| February 19 | 15:30:16.00 | 29.9897 | 24.19 | 4x523 | 235 | 8.8 | −77.9 ± 11.7 | 3.94 ± 0.07 | 3915 ± 3 |
| February 20 | 15:45:20.56 | 31.0002 | 25.00 | 4x523 | 210 | 9.1 | −73.6 ± 13.4 | 4.36 ± 0.06 | 3908 ± 3 |
| February 21 | 14:10:33.49 | 31.9344 | 25.75 | 4x523 | 268 | 8.1 | −87.5 ± 11.0 | 3.77 ± 0.07 | 3934 ± 3 |
| February 22 | 14:43:39.96 | 32.9574 | 26.58 | 4x523 | 275 | 7.5 | −86.4 ± 10.5 | 3.43 ± 0.07 | 3955 ± 3 |
| February 25 | 13:37:16.21 | 35.9112 | 28.96 | 4x523 | 251 | 8.7 | −40.4 ± 12.8 | 4.39 ± 0.08 | 3911 ± 3 |
| February 26 | 14:24:21.07 | 36.9439 | 29.79 | 4x523 | 227 | 8.8 | −71.9 ± 12.0 | 3.79 ± 0.06 | 3930 ± 3 |
| February 27 | 13:31:08.50 | 37.9070 | 30.57 | 4x523 | 213 | 8.7 | −75.2 ± 12.6 | 3.40 ± 0.07 | 3953 ± 3 |
| March 02 | 13:37:56.10 | 41.9117 | 33.80 | 4x523 | 278 | 7.7 | −64.5 ± 10.8 | 3.84 ± 0.07 | 3932 ± 3 |
The columns are: (1 and 2) date and universal time of the observations, (3) heliocentric Julian date, (4) rotational cycle of the observations found using Eq. 1, (5) exposure time of a polarimetric sequence, (6) signal-to-noise ratio at 1650 nm per polarimetric sequence, (7) RMS noise level of Stokes V signal in units of unpolarised continuum, (8) longitudinal magnetic field (see Eq 3) with error bar estimated from formal propagation, (9) average unsigned magnetic field, and (10) effective surface temperature.
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