| | 1 | 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. |
| | 2 | |
| | 3 | |
| | 4 | || exp_id || dateobs || moon_angle || moon_phase || |
| | 5 | || 94818 || 2009-09-06 10:02:30 || 19.9828 || 0.547319 || |
| | 6 | || 94822 || 2009-09-06 10:08:51 || 24.5752 || 0.547387 || |
| | 7 | || 94826 || 2009-09-06 10:15:03 || 32.6811 || 0.547452 || |
| | 8 | || 94828 || 2009-09-06 10:18:16 || 19.8979 || 0.547486 || |
| | 9 | || 94833 || 2009-09-06 10:26:19 || 36.004 || 0.547569 || |
| | 10 | || 94835 || 2009-09-06 10:29:37 || 31.0689 || 0.547603 || |
| | 11 | |
