DataLabel | Date Time | Log Entry |
---|---|---|
GN-2006A-Q-75-130-001 | 2006-04-08 11:59:52 | Saturated - observer thought Texp was 15 sec not 30 sec. |
GN-2006A-Q-75-130-002 | 2006-04-08 12:01:36 | Saturated - peak=29849 |
GN-2006A-Q-75-130-003 | 2006-04-08 12:02:48 | peak=24196 |
GN-2006A-Q-75-130-004 | 2006-04-08 12:04:06 | peak=32705 |
GN-2006A-Q-75-130-005 | 2006-04-08 12:05:18 | peak=24653 |
GN-2006A-Q-75-130-006 | 2006-04-08 12:06:51 | Changed to 3 x 10 sec coadds. Peak = 31594. Three of the five images in this repeated sequence have at least a few pixels above non-linearity (30000) so I have marked the whole observation USABLE and it will have to be repeated. But the images should be distributed because they can be useful to the PI maybe. |
GN-2006A-Q-75-130-007 | 2006-04-08 12:07:34 | Peak=24543, FWHM=0.126", looks quite round to me though (imexam contours). |
GN-2006A-Q-75-130-008 | 2006-04-08 12:08:27 | Peak=25331 |
GN-2006A-Q-75-130-009 | 2006-04-08 12:09:10 | Peak=30665 |
GN-2006A-Q-75-130-010 | 2006-04-08 12:09:58 | Peak=35384. NB Altair seeing dropped steadily over the course of these observations from about 0.8" with fluctuations as high as 0.96", ending up at about 0.65" at end of PSF star. |