Changes between Version 8 and Version 9 of docs/CommissioningPlan/P3.11
- Timestamp:
- 04/22/22 20:49:58 (3 years ago)
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docs/CommissioningPlan/P3.11
v8 v9 1 == P3.11 Sky background==2 1 == P3.11 Astrometry plate scale and orientation == 2 3 3 - **Phase** : 3 4 4 - **Status** : Draft 5 5 - **Category** : Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6) 6 - **Recurrence** : once at commissioning and then on request.6 - **Recurrence** : every night starting from commissioning 7 7 - **Duration** : 2 hours 8 8 9 9 **Description** 10 - Acquire a series of sky backgrounds from science images. A short sky background may also be useful for remaining deviant pixel removal.10 - Determine the astrometry of the science frame. Deduce detector on sky coordinates & plate scale from RA & DEC of known multiple stellar systems. This calibration is to be done for a reference setup. 11 11 12 12 **Prerequisites** 13 13 - Authorize SHARK-NIR on the SX side. 14 - Atmospheric conditions: AO working conditions??? 14 - Atmospheric conditions: AO working conditions. 15 - Bad pixel map, Background or Dark, Flat-field, distortion map 15 16 16 17 **Procedure** 17 - Observe a blank field close to the science target (separation~10-20 arcsec) 18 - The same set-up as nighttime science observations, but AO is not running, and the coronagraph may be removed. A list of telescope offsets is added to reach an “empty” field and jitter. 18 - Observe multiple systems with known characteristics without the coronagraph 19 19 20 20 **Templates** 21 - SHARKNIR_cal_ SkyBackground(not released)21 - SHARKNIR_cal_Astrometry (not released) 22 22 23 23 **Success criteria** 24 - 10% accuracy (dependent on measurement frequency)24 - Image scale better than 5 mas (goal 0.5 mas) over FoV, image orientation better than 3 arcmins (goal 18 arcsec) 25 25 26 26 **Notes** 27 - Same as activity 7. 6in AD427 - Same as activity 7.1 in AD4 28 28 29 29 **LBTO support** 30 - AO support 30 31 31 32 **Date performed and by whom**