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Table 2
Dates, UT, separation between the star and the phase centre, rms measured on the map and rotational phase of the star corresponding to the middle of the observation run for BP Boo.
Date | UT | Separation (deg) | rms S1 (mJy) | Rot. phase |
---|---|---|---|---|
2017 Oct. 14 | 11:00 | 0.36 | 0.06 | 0.45 |
2020 Mar. 14 | 23:49 | 2.30 | 0.17 | 0.63 |
2016 Mar. 11 | 00:08 | 2.34 | 0.14 | 0.88 |
2019 Dec. 02 | 07:11 | 2.77 | 0.30 | 0.59 |
2016 Apr. 07 | 22:10 | 2.90 | 0.21 | 0.43 |
2020 May24 | 19:20 | 3.16 | 0.37 | 0.29 |
2020 May11 | 20:01 | 3.42 | 0.60 | 0.27 |
2016 Mar. 03 | 00:23 | 3.69 | 0.54 | 0.71 |
Notes. The rotational phase was computed using the rotational period and reference epoch in Sikora et al. (2019b).
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