Table 3.

Log of spectroscopic observations of HIP 71933 for our epochs. The first two columns list the epoch of the observation and telescope. Column 3 lists the instrument resolution. Columns 4, 5, and 6 list the date, start time, and end time for the exposures. Column 7 lists the number of usable exposures in the sequence. Column 7 lists the rotational cycles for each epoch from the first to last exposure. The zero phase was calculated to be the mid-point of the first epoch and is at JD 245 4932.2110 (see equation 1). The zero-points for all subsequent epochs are calculated as an integer number of rotations starting with the zero-point of the first epoch that is the closest to the mid-point of each epoch.

EpochTelescopeInstrument resolutionDateut startut endNo. Stokes I exposuresRotational cycle
2009.26AAT∼70 0002009 Apr 0712:2016:028−4.563 to 4.668
2009 Apr 0811:0116:4512
2009 Apr 0911:4018:227
2009 Apr 1316:1116:554
2009.342.3-m∼24 0002009 May 0412:3917:367−1.214 to 2.070
2009 May 0610:3510:5511
2010.332.3-m∼24 0002010 Apr 0112:0918:5915−2.722 to 2.093
2010 Apr 0212:3819:1311
2010 Apr 0313:0517:1610
2010 Apr 0412:2217:209
2011.373.6-m∼115 0002011 May 1602:0423:2012−3.384 to 4.147
2011 May 1701:3923:1912
2011 May 1800:2623:5716
2011 May 1901:1707:318
2011 May 2000:0123:2822
2012.262.3-m∼24 0002012 Apr 0412:2816:595−4.180 to 3.596
2012 Apr 0515:1118:443
2012 Apr 0616:2917:302
2012 Apr 0711:1517:416
2012 Apr 0911:5117:416
2018.072.3-m∼24 0002018 Jan 2516:4518:374−2.763 to 1.794
2018 Jan 2815:1618:066
2019.462.3-m∼24 0002019 June 1708:0711:4610−2.080 to 2.874
2019 June 1808:0412:1612
2019 June 1908:0516:0616
2019 June 2008:0216:0218
EpochTelescopeInstrument resolutionDateut startut endNo. Stokes I exposuresRotational cycle
2009.26AAT∼70 0002009 Apr 0712:2016:028−4.563 to 4.668
2009 Apr 0811:0116:4512
2009 Apr 0911:4018:227
2009 Apr 1316:1116:554
2009.342.3-m∼24 0002009 May 0412:3917:367−1.214 to 2.070
2009 May 0610:3510:5511
2010.332.3-m∼24 0002010 Apr 0112:0918:5915−2.722 to 2.093
2010 Apr 0212:3819:1311
2010 Apr 0313:0517:1610
2010 Apr 0412:2217:209
2011.373.6-m∼115 0002011 May 1602:0423:2012−3.384 to 4.147
2011 May 1701:3923:1912
2011 May 1800:2623:5716
2011 May 1901:1707:318
2011 May 2000:0123:2822
2012.262.3-m∼24 0002012 Apr 0412:2816:595−4.180 to 3.596
2012 Apr 0515:1118:443
2012 Apr 0616:2917:302
2012 Apr 0711:1517:416
2012 Apr 0911:5117:416
2018.072.3-m∼24 0002018 Jan 2516:4518:374−2.763 to 1.794
2018 Jan 2815:1618:066
2019.462.3-m∼24 0002019 June 1708:0711:4610−2.080 to 2.874
2019 June 1808:0412:1612
2019 June 1908:0516:0616
2019 June 2008:0216:0218
Table 3.

Log of spectroscopic observations of HIP 71933 for our epochs. The first two columns list the epoch of the observation and telescope. Column 3 lists the instrument resolution. Columns 4, 5, and 6 list the date, start time, and end time for the exposures. Column 7 lists the number of usable exposures in the sequence. Column 7 lists the rotational cycles for each epoch from the first to last exposure. The zero phase was calculated to be the mid-point of the first epoch and is at JD 245 4932.2110 (see equation 1). The zero-points for all subsequent epochs are calculated as an integer number of rotations starting with the zero-point of the first epoch that is the closest to the mid-point of each epoch.

EpochTelescopeInstrument resolutionDateut startut endNo. Stokes I exposuresRotational cycle
2009.26AAT∼70 0002009 Apr 0712:2016:028−4.563 to 4.668
2009 Apr 0811:0116:4512
2009 Apr 0911:4018:227
2009 Apr 1316:1116:554
2009.342.3-m∼24 0002009 May 0412:3917:367−1.214 to 2.070
2009 May 0610:3510:5511
2010.332.3-m∼24 0002010 Apr 0112:0918:5915−2.722 to 2.093
2010 Apr 0212:3819:1311
2010 Apr 0313:0517:1610
2010 Apr 0412:2217:209
2011.373.6-m∼115 0002011 May 1602:0423:2012−3.384 to 4.147
2011 May 1701:3923:1912
2011 May 1800:2623:5716
2011 May 1901:1707:318
2011 May 2000:0123:2822
2012.262.3-m∼24 0002012 Apr 0412:2816:595−4.180 to 3.596
2012 Apr 0515:1118:443
2012 Apr 0616:2917:302
2012 Apr 0711:1517:416
2012 Apr 0911:5117:416
2018.072.3-m∼24 0002018 Jan 2516:4518:374−2.763 to 1.794
2018 Jan 2815:1618:066
2019.462.3-m∼24 0002019 June 1708:0711:4610−2.080 to 2.874
2019 June 1808:0412:1612
2019 June 1908:0516:0616
2019 June 2008:0216:0218
EpochTelescopeInstrument resolutionDateut startut endNo. Stokes I exposuresRotational cycle
2009.26AAT∼70 0002009 Apr 0712:2016:028−4.563 to 4.668
2009 Apr 0811:0116:4512
2009 Apr 0911:4018:227
2009 Apr 1316:1116:554
2009.342.3-m∼24 0002009 May 0412:3917:367−1.214 to 2.070
2009 May 0610:3510:5511
2010.332.3-m∼24 0002010 Apr 0112:0918:5915−2.722 to 2.093
2010 Apr 0212:3819:1311
2010 Apr 0313:0517:1610
2010 Apr 0412:2217:209
2011.373.6-m∼115 0002011 May 1602:0423:2012−3.384 to 4.147
2011 May 1701:3923:1912
2011 May 1800:2623:5716
2011 May 1901:1707:318
2011 May 2000:0123:2822
2012.262.3-m∼24 0002012 Apr 0412:2816:595−4.180 to 3.596
2012 Apr 0515:1118:443
2012 Apr 0616:2917:302
2012 Apr 0711:1517:416
2012 Apr 0911:5117:416
2018.072.3-m∼24 0002018 Jan 2516:4518:374−2.763 to 1.794
2018 Jan 2815:1618:066
2019.462.3-m∼24 0002019 June 1708:0711:4610−2.080 to 2.874
2019 June 1808:0412:1612
2019 June 1908:0516:0616
2019 June 2008:0216:0218
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