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Table A.1

Journal of observations.

Date Mid-HJD Star Texp (s) S / N

17 Mar. 2010 2 455 273.520 β UMa 16 × 4 × 107 52 707 ± 6090
06 Apr. 2010 2 455 293.412 β UMa 17 × 4 × 107 49 436 ± 22 333
10 Apr. 2010 2 455 297.444 β UMa 19 × 4 × 107 76 493 ± 1960
11 Apr. 2010 2 455 298.397 β UMa 19 × 4 × 107 32 500 ± 7752
25 Mar. 2011 2 455 646.426 β UMa 25 × 4 × 107 56 378 ± 24 444
31 Mar. 2011 2 455 652.504 β UMa 25 × 4 × 107 45 963 ± 4907
02 Apr. 2011 2 455 654.379 β UMa 03 × 4 × 107 53 964 ± 8998
04 Apr. 2011 2 455 656.462 β UMa 24 × 4 × 107 69 029 ± 6099
22 Jan. 2012 2 455 949.644 θ Leo 05 × 4 × 180 44 503 ± 1018
23 Jan. 2012 2 455 950.628 θ Leo 05 × 4 × 180 39 774 ± 5090
24 Jan. 2012 2 455 951.624 θ Leo 05 × 4 × 180 41 547 ± 3889
25 Jan. 2012 2 455 952.640 θ Leo 05 × 4 × 180 41 737 ± 3134
14 Mar. 2012 2 456 001.579 θ Leo 05 × 4 × 180 43 929 ± 1810
15 Mar. 2012 2 456 002.524 θ Leo 10 × 4 × 180 47 360 ± 698
24 Mar. 2012 2 456 011.526 θ Leo 05 × 4 × 180 44 880 ± 1487
25 Mar. 2012 2 456 012.502 θ Leo 05 × 4 × 180 47 392 ± 506
27 Mar. 2012 2 456 013.400 θ Leo 10 × 4 × 180 40 883 ± 1229
21 Mar. 2013 2 456 373.488 θ Leo 09 × 4 × 180 25 542 ± 4619
23 Mar. 2013 2 456 375.465 θ Leo 09 × 4 × 180 29 220 ± 2557
16 Apr. 2013 2 456 399.444 θ Leo 09 × 4 × 180 23 751 ± 3600
17 Apr. 2013 2 456 400.492 θ Leo 09 × 4 × 180 45 010 ± 1529
22 Apr. 2013 2 456 405.512 θ Leo 09 × 4 × 180 42 777 ± 1707
23 Apr 2013 2 456 406.454 θ Leo 09 × 4 × 180 42 064 ± 2815
24 Apr. 2013 2 456 407.502 θ Leo 09 × 4 × 180 39 578 ± 2497
14 Apr. 2014 2 456 762.445 θ Leo 05 × 4 × 180 25 433 ± 8566
07 May 2014 2 456 785.408 θ Leo 05 × 4 × 180 42 839 ± 3748
08 May 2014 2 456 786.411 θ Leo 05 × 4 × 180 39 435 ± 2842
09 May 2014 2 456 787.416 θ Leo 05 × 4 × 180 44 236 ± 617
14 May 2014 2 456 792.471 θ Leo 05 × 4 × 180 42 041 ± 543
15 May 2014 2 456 793.413 θ Leo 05 × 4 × 180 44 653 ± 1052
07 Jun. 2014 2 456 816.408 θ Leo 05 × 4 × 180 29 599 ± 1530
10 Jun. 2014 2 456 819.415 θ Leo 05 × 4 × 180 29 931 ± 3928

Notes. The columns contain the date for each Stokes V sequence, the heliocentric Julian date corresponding to the middle of the observation time, the object name, the number of sequences, the exposure time per individual subexposure and the averaged S/N in the individual LSD Stokes V pseudo-line profiles (±rms).

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