Monte-Carlo simulation of ELT scale multi-object adaptive optics deformable mirror requirements and tolerances
A. G. Basden, N. A. Bharmal, R. M. Myers, S. L. Morris, T. J. Morris

TL;DR
This study uses Monte-Carlo simulations to determine deformable mirror requirements and tolerances for multi-object adaptive optics on extremely large telescopes, highlighting potential cost savings and performance considerations.
Contribution
It provides a detailed analysis of DM actuator density, stroke, and alignment tolerances for MOAO systems using end-to-end simulations, considering ground-layer correction effects.
Findings
Actuator density can be reduced with minimal performance loss when using a ground-layer DM.
Maximum DM stroke requirement is quantified at 3.5 μm.
Alignment tolerances are specified for lateral and rotational positioning.
Abstract
Multi-object adaptive optics (MOAO) has been demonstrated by the CANARY instrument on the William Herschel Telescope. However, for proposed MOAO systems on the next generation Extremely Large Telescopes, such as EAGLE, many challenges remain. Here we investigate requirements that MOAO operation places on deformable mirrors (DMs) using a full end-to-end Monte-Carlo AO simulation code. By taking into consideration a prior global ground-layer (GL) correction, we show that actuator density for the MOAO DMs can be reduced with little performance loss. We note that this reduction is only possible with the addition of a GL DM, whose order is greater than or equal to that of the original MOAO mirrors. The addition of a GL DM of lesser order does not affect system performance (if tip/tilt star sharpening is ignored). We also quantify the maximum mechanical DM stroke requirements (3.5 m…
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