Changes between Version 7 and Version 8 of docs/CommissioningPlan/P3.6
- Timestamp:
- 01/14/22 18:47:09 (3 years ago)
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docs/CommissioningPlan/P3.6
v7 v8 1 == P3.6 PSF Alignment == 2 • **Phase** : 3 3 • **Status** : Draft 4 • **Category** : Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6) 5 • **Recurrence** : before every observing target (CI, LSS), starting from commissioning. 6 • **Duration** : 2 hours 1 == P3.6 Verify the ADC rotation on sky == 2 3 - **Phase** : 3 4 - **Status** : Draft 5 - **Category** : Nighttime testing (functionality and operability) (C5) 6 - **Recurrence** : once at commissioning 7 - **Duration** : 1 night 8 7 9 **Description** 8 • Alignment of the PSF with occulter (or slit) in coronagraphic mode. 10 - Evaluate the performance of the SHARK-NIR ADC. 11 9 12 **Prerequisites** 10 • Bad pixel map, Background or Dark, Flat-field, detector RON 13 - Atmospheric conditions: photometric. 14 - Authorize SHARK-NIR on the SX side. 15 - Photometric stars as targets for every filter. 16 - AO is working. 17 - Target(s) at different Zenith distances? 18 11 19 **Procedure** 12 • The position of the internal deformable mirror (TTM_DM) is optimized in order to have the PSF image on the intermediate focal plane centered with the occulter. This is obtained comparing the PSF image, formed on the SCICAM, with the image of the occulter, obtained on the SCICAM using the calibration flat-field source. 20 - Check the working of the ADC using different targets in varying zenith distances and observing using different science filters? 21 22 **Templates** 23 13 24 **Success criteria** 14 • the expected accuracy of 0.2 pixels (DV: need to check if we can reach this). 25 - xxx 26 15 27 **Notes** 16 • Same as activity 8.3 in AD4 17 * 7 cases, 30 mins per case. 28 18 29 **LBTO support** 19 • AO support 20 **Associated SHARK-NIR personnel** 30 - AO support 21 31 22 32 **Date performed and by whom**