Changes between Version 9 and Version 10 of docs/CommissioningPlan/P3.1
- Timestamp:
- 12/08/22 02:52:03 (2 years ago)
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docs/CommissioningPlan/P3.1
v9 v10 9 9 **Description** 10 10 - Preset of a bright enough on-axis star is sent to the telescope for verifying the communication to TCS, nighttime collimation model for SHARK-NIR, and the pointing accuracy. 11 - For the correct telescope mode for SHARK-NIR, find the offset direction & magnitude (for the field-stabilized mode), verify the proper image orientation , pixel scale, field of view, and distortionat the SCICAM. Note that this may be performed with and without AO running.11 - For the correct telescope mode for SHARK-NIR, find the offset direction & magnitude (for the field-stabilized mode), verify the proper image orientation at the SCICAM. Note that this may be performed with and without AO running. 12 12 13 13 … … 32 32 - Issue a preset to move to a suitable astrometric binary (typically 5-8 arcsec separation) and center one star in the science channel. 33 33 - Based on the published coordinates of the binary, issue the appropriate offset to center the other star. 34 3. Procedure for pixel scale/ plate scale 35 - Select a filter 36 - Issue a preset to move to a suitable astrometric binary to measure pixel scale (typically 5-8 arcsec separation) 37 - Center the binary in the upper half of the SCICAM and take several frames. Average these frames 38 - Move the binary to the lower half of the SCICAM and repeat. 39 - Use the difference image (optionally flat-fielded) to verify the expected pixel scale. This gives two measures. 40 - Repeat this for other filters. 34 41 35 **Templates** 42 36 - Tel_Target_Acq … … 46 40 **Success criteria** 47 41 - Successful in sending preset to the telescope and, therefore, communication with LBT TCS. 48 - The image orientation is as expected. The pixel scale and field of view of the SCICAM are as expected.42 - The image orientation is as expected. 49 43 **Notes** 50 44