== P3.4 Telescope control – telescope mode, offset, and focal plane geometry estimation== • **Phase** : 3 • **Status** : Draft • **Category** : Nighttime testing (functionality and operability) (C4) • **Recurrence** : once at commissioning • **Duration** : 1 night **Description** • 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 distortion at the SCICAM. Note that this may be performed with and without AO running. **Prerequisites** • Atmospheric conditions: should be able to see bight stars on sky (preferably close to zenith?). • Authorize SHARK-NIR on the SX side. • Suitable binary or astrometric targets. • AO running for part of the test. **Procedure** 1. **Procedure** for image orientation - Select a filter - Place the de-rotator in the nominal "zero" position. - Issue a preset to move to a bright star (but not too bright to saturate) - Center the star in the science channel - Issue a pure elevation offset to the TCS of ca. 5” and verify expected motion direction on the SCICAM - Return to the on-axis position and repeat with a pure azimuth motion. - Issue a preset to move to a suitable astrometric binary (typically 5-8 arcsec separation) and center one star in the science channel. - Based on the published coordinates of the binary, issue the appropriate offset to center the other star. 2. **Procedure** for pixel scale/ plate scale - Select a filter - Issue a preset to move to a suitable astrometric binary to measure pixel scale (typically 5-8 arcsec separation) - Center the binary in the upper half of the SCICAM and take several frames. Average these frames - Move the binary to the lower half of the SCICAM and repeat. - Use the difference image (optionally flat-fielded) to verify the expected pixel scale. This gives two measures. - Repeat this for other filters. **Success criteria** • The image orientation is as expected. The pixel scale and field of view of the SCICAM are as expected. **Notes** **LBTO support** • Support from telescope operator (if needed). • Presence of John Hill usually helps while collimating for the first time. **Associated SHARK-NIR personnel** **Date performed and by whom**