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Table 3

Journal of observations for 2007.59, 2008.09, and 2009.46.

Year Julian date σLSD Rot. phase
(2 450 000+) 10-5Ic

2007.59 4308.35 5.4742 0.8726
4310.35 1.7360 0.1835
4311.35 2.1059 0.3387
4312.34 2.7435 0.4928
4313.34 3.8929 0.6485
4315.34 2.8654 0.9586
4316.34 2.7608 0.1152
4322.34 3.2082 0.0473
4323.34 3.7479 0.2030

2008.09 4484.72 5.9851 0.3017
4484.77 6.3988 0.3092
4485.77 5.2155 0.4648
4488.76 3.2560 0.9291
4489.74 3.4732 0.0827
4489.75 3.5767 0.0840
4491.70 4.0728 0.3865
4492.75 3.3416 0.5499
4493.76 2.7275 0.7075
4495.77 3.4875 0.0206
4499.77 12.7455 0.6427
4501.77 3.5052 0.9538
4503.76 3.1664 0.2626
4506.77 2.9219 0.7304
4507.76 1.3428 0.8843
4508.76 4.5386 0.0400
4509.73 7.8197 0.1914
4510.77 4.1865 0.3524
4512.76 3.1274 0.6627

2009.46 4980.38 4.0385 0.3865
4984.45 12.1589 0.0192
4985.43 3.7381 0.1722
4994.47 5.3269 0.5786
4995.46 4.3773 0.7318
5001.44 14.4977 0.6617
5002.36 10.5647 0.8056
5006.56 3.2475 0.4579
5010.46 5.4779 0.0654
5011.44 4.6241 0.2175
5013.55 4.3254 0.5450
5017.38 6.9613 0.1415
5018.40 3.1676 0.2992

Notes. From left to right, we list the year of observation, the Julian date, the error-bar in Stokes V LSD profiles, and the phase of the rotational cycle at which the observation was made, taking the same rotation period and phase origin as Petit et al. (2005).

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