Changes between Version 2 and Version 3 of docs/CommissioningPlan/P3.19
- Timestamp:
- 01/19/21 17:50:45 (4 years ago)
Legend:
- Unmodified
- Added
- Removed
- Modified
-
docs/CommissioningPlan/P3.19
v2 v3 1 == P3.1 9 Distortion map==1 == P3.14 Sky background == 2 2 • **Phase** : 3 3 3 • **Status** : Draft 4 • **Category** : Nighttime calibration (C5)5 • **Recurrence** : once every week starting from commissioning +on request.4 • **Category** : Nighttime testing (functionality and operability) (C4) 5 • **Recurrence** : once at commissioning and then on request. 6 6 • **Duration** : 1 hour 7 7 **Description** 8 • Determine distortion map of science frame. Monitor distortion coefficient with time (weekly calibration) and measure the precise distortion of a given observation in any setup, if requested.8 • Acquire a series of sky backgrounds from science images, expected mainly when observing extended objects. A short sky background may also be useful for remaining deviant pixel removal. 9 9 **Prerequisites** 10 10 • Authorize SHARK-NIR on the SX side. 11 • Atmospheric conditions: AO working conditions. 12 • Bad pixel map, Background or Dark, Flat-field, distortion map 11 • Atmospheric conditions: AO working conditions??? 13 12 **Procedure** 14 • Observe a dense field (e.g., a globular cluster) with accurate HST astrometry and a guide star bright enough (mag F860W < 11). 13 • Observe a blank field close to the science target (separation~10-20 arcsec) 14 • The same set-up as normal science observations but AO is not running and coronagraph may be removed. A list of telescope offsets is added to reach an “empty” field and jitter. 15 15 **Success criteria** 16 • Better than 1 mas over FoV.16 • 10% accuracy (dependent on measurement frequency) 17 17 **Notes** 18 • Same as activity 9.6 in AD418 • Same as activity 7.6 in AD4 19 19 **LBTO support** 20 20 • SOUL-AO support 21 22 21 **Associated SHARK-NIR personnel** 23 22 24 25 23 **Date performed and by whom**