Table 1: Journal of observations.
Star UT date and time $\phi^{*}$ Config. B [m] PA [deg]
$\pi ^{1}$ Gruis 2006-05-21 09:09:26 ... E0-G0 15.7 50
$\beta $ Gruis 2006-05-21 09:28:33 0.23 - - -
$\pi ^{1}$ Gruis 2006-05-23 09:32:27 ... A0-G0 63.5 56
$\beta $ Gruis 2006-05-23 10:06:51 0.28 - - -
$\pi ^{1}$ Gruis 2006-05-24 09:27:34 ... D0-G0 31.8 56
$\beta $ Gruis 2006-05-24 09:44:39 0.31 - - -
$\pi ^{1}$ Gruis 2006-05-25 08:09:13 ... A0-G0 61.2 41
$\beta $ Gruis 2006-05-25 07:51:28 0.34 - - -
$\pi ^{1}$ Gruis 2006-05-27 09:20:41 ... E0-G0 15.9 57
$\beta $ Gruis 2006-05-27 09:37:11 0.39 - - -
$\pi ^{1}$ Gruis 2006-06-19 10:16:01 ... D0-G0 30.6 83
$\beta $ Gruis 2006-06-19 09:50:14 0.01 - - -
$\pi ^{1}$ Gruis 2006-08-08 08:40:43 ... A0-G0 52.6 102
$\beta $ Gruis 2006-08-08 08:13:56 0.36 - - -
* The pulsation phase for $\beta $ Gruis (Otero & Moon 2006). This was not possible
for $\pi ^{1}$ Gruis due to the non-regular character of its lightcurve.

Source LaTeX | All tables | In the text