High precision optical instruments are set to deliver GAIA-quality astrometric precision. In order to reach these demanding goals, it is crucial to calibrate the optical instruments themselves to an even higher level of precision. This project aims to research and potentially develop the design of calibration light sources for use in the MAVIS instrument (currently being designed for the ESO VLT). The calibration sources must satisfy a strict set of requirements, such as repeatability, flux throughput, and the ability to be reconfigured on demand.

A student undertaking this project should achieve the following learning outcomes:

1. Proficiency in designing and implementing precise calibration methods.

2. Understanding of the key requirements for accurate calibration in optical instruments.

3. Skill development in researching and evaluating calibration strategies.

4. Application of calibration techniques to optimize instrument performance.

Experience in opto-mechanical design and instrumentation is highly valued.