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Table 5
Observing log of Doppler-imaging sets.
| Set | Year | HJD range | N | Max. phase | rms |
| (2 450 000+) | gap | ||||
|
|
|||||
| 1 | 2009.28 | 4923−4944 | 15 | 0.13 | 0.0196 |
| 2 | 2009.52 | 5009−5033 | 25 | 0.05 | 0.0021 |
| 3 | 2009.59 | 5033−5059 | 25 | 0.07 | 0.0022 |
| 4 | 2009.67 | 5060−5089 | 25 | 0.09 | 0.0020 |
| 5 | 2010.45 | 5348−5370 | 13 | 0.27 | 0.0019 |
| 6 | 2010.53 | 5377−5400 | 14 | 0.14 | 0.0020 |
| 7 | 2010.59 | 5401−5419 | 10 | 0.20 | 0.0024 |
| 8 | 2010.67 | 5429−5451 | 17 | 0.13 | 0.0019 |
| 9 | 2010.73 | 5452−5476 | 10 | 0.31 | 0.0017 |
| 10 | 2010.81 | 5478−5507 | 12 | 0.47 | 0.0018 |
| 11 | 2011.36 | 5685−5699 | 7 | 0.38 | 0.0018 |
| 12 | 2011.47 | 5722−5742 | 17 | 0.13 | 0.0020 |
| 13 | 2011.53 | 5743−5763 | 12 | 0.26 | 0.0020 |
Notes. The year is given for the mid-times of the related sets. N is the number spectra per set, and max-phase gap is the largest rotational phase gap between two successive observation. The error value of each inverted set is given in the rms column.
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