In an attempt to find a way for the IPP to identify which exposures show moon glints, I examined a series of Three Pi exposures that had small moon angles and had visible glint features.  All exposures are in the i filter.

|| exp_id || dateobs             || moon_angle || moon_phase ||
||  94818 || 2009-09-06 10:02:30 ||    19.9828 ||   0.547319 ||
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||[[Image(94818.jpeg, 700px)]] || [[Image(o5080g0156ojt.jpeg, 700px)]]
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|| exp_id || dateobs             || moon_angle || moon_phase ||
||  94822 || 2009-09-06 10:08:51 ||    24.5752 ||   0.547387 || 
[[Image(94822.jpeg, 600px)]]
|| exp_id || dateobs             || moon_angle || moon_phase ||
||  94826 || 2009-09-06 10:15:03 ||    32.6811 ||   0.547452 || 
[[Image(94826.jpeg, 800px)]]
|| exp_id || dateobs             || moon_angle || moon_phase ||
||  94828 || 2009-09-06 10:18:16 ||    19.8979 ||   0.547486 || 
[[Image(94828.jpeg, 800px)]]
|| exp_id || dateobs             || moon_angle || moon_phase ||
||  94833 || 2009-09-06 10:26:19 ||     36.004 ||   0.547569 || 
[[Image(94833.jpeg, 800px)]]
|| exp_id || dateobs             || moon_angle || moon_phase ||
||  94835 || 2009-09-06 10:29:37 ||    31.0689 ||   0.547603 || 
[[Image(94835.jpeg, 800px)]]