Changes between Version 8 and Version 9 of docs/CommissioningPlan/P3.13
- Timestamp:
- 01/14/22 18:59:15 (3 years ago)
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docs/CommissioningPlan/P3.13
v8 v9 1 == P3.13 Center the slit == 2 • **Phase** : 3 3 • **Status** : Draft 4 • **Category** : Nighttime testing (functionality and operability) (C5) 5 • **Recurrence** : once at commissioning 6 • **Duration** : 2 nights 1 == P3.13 Distortion map == 2 3 - **Phase** : 3 4 - **Status** : Draft 5 - **Category** : Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6) 6 - **Recurrence** : once every week starting from commissioning + on request. 7 - **Duration** : 4 hours 8 7 9 **Description** 8 • This activity will center the long slit. 10 - 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. 11 9 12 **Prerequisites** 10 • Atmospheric conditions: AO working conditions. 11 • Authorize SHARK-NIR on the SX side. 13 - Authorize SHARK-NIR on the SX side. 14 - Atmospheric conditions: AO working conditions. 15 - Bad pixel map, Background or Dark, Flat-field, distortion map 16 12 17 **Procedure** 13 • Point to known binary stars and then offset the telescope and the rotators to get to the nominal (known) position of the planet or introducing a bright speckle by using secondary mirrors at the same parallactic angle of the planet in order to align the slit. 14 * TBD 18 - Observe a dense field (e.g., a globular cluster) with accurate HST astrometry and a guide star bright enough (mag F860W < 11). 19 20 **Templates** 21 15 22 **Success criteria** 16 • xxx 23 - Better than 1 mas over FoV. 24 17 25 **Notes** 26 - Same as activity 9.6 in AD4 18 27 19 28 **LBTO support** 20 • AO support 21 **Associated SHARK-NIR personnel** 29 - AO support 22 30 23 31 **Date performed and by whom** 24 25 ** Comments**