Changes between Version 3 and Version 4 of docs/CommissioningPlan/P1.11
- Timestamp:
- 02/03/21 17:50:29 (4 years ago)
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docs/CommissioningPlan/P1.11
v3 v4 1 == P1.11 Check the working of the internal NCPA routine and looking for filter defects/artifacts == 2 • **Phase** : 2 1 2 == P1.11 Science detector calibrations == 3 • **Phase** : 1 3 4 • **Status** : Draft 4 • **Category** : Unpack, Assemble, and Verification (C1) ???5 • **Recurrence** : once at commissioning5 • **Category** : Unpack, Assemble, and Verification (C1) ??? 6 • **Recurrence** : once 6 7 • **Duration** : 1 day 7 8 **Description** 8 • Check the working of the internal NCPA routine. Finding the filter defects/artifacts using an internal calibration source (flat-field) within the instrument. 9 • Calibration and testing of the SHARK-NIR science detector 10 **Prerequisites** 11 • SHARK-NIR connected to LBT network. 12 • Electronics cabinets on. 13 • The cryostat should be running and cooled down. 14 • Internal alignment of the SHARK-NIR is verified. 15 **Procedure** 16 • check bias calibration & master dark scripts and then perform the following daytime calibration procedures below. 9 17 10 **Prerequisites** 11 • SCICAM cooled down. 18 ||SDC1||[wiki:/docs/CommissioningPlan/SDC1 Instrumental background for science]|| 19 ||SDC2||[wiki:/docs/CommissioningPlan/SDC2 Instrument flat field, detector linearity and bad pixels]|| 20 ||SDC3||[wiki:/docs/CommissioningPlan/SDC3 Wavelength calibration]|| 21 ||SDC4||[wiki:/docs/CommissioningPlan/SDC4 Thermal background]|| 22 ||SDC5||[wiki:/docs/CommissioningPlan/SDC5 Detector gain]|| 23 ||SDC6||[wiki:/docs/CommissioningPlan/SDC6 Detector persistence]|| 24 ||SDC7||[wiki:/docs/CommissioningPlan/SDC7 Spectral resolution]|| 25 ||SDC8||[wiki:/docs/CommissioningPlan/SDC8 Ghost calibration]|| 12 26 13 **Procedure** 14 • Run the Phase-diversity routine using the images taken with the SHARK-NIR internal calibration sources to measure the NCPA within (excluding the deployable arm) 15 * Take the images of all the filters using the internal calibration source (flat-field) within the instrument to locate/find out the filter defects/artifacts, if any. 16 • You may take short- and long-exposures to get better contrast of the features if required. 27 * Check the working of all the detector read-out modes and windowing possibilities. 17 28 18 29 **Success criteria** 19 * Internal NCPA routine works fine and the PSF shows improvement in its quality. 20 • All the filter images saved. 30 • linearity as expected 31 • bad pixels mask created 32 • bias and flat took 33 * All individual activity (in the table) success criteria is met 21 34 **Notes** 22 • The time dedicated to this activity has to be considered in combination with the other activities if needed. Parallelism is possible.35 • Save all the intermediate images to check the SHARK-NIR Data Reduction pipeline. 23 36 **LBTO support** 24 37 … … 28 41 29 42 **Comments** 30 31 * KR: add the filter monitoring routine check. 43 * MB: not sure about all these. It should already take place in Padova. For sure bias offset will be recomputed at these elevation due to different temperature than can be reached