Paper
12 July 2018 LO WFS of MAORY: performance and sky coverage assessment
Author Affiliations +
Abstract
MAORY is the Multi-Conjugate Adaptive Optics module for the European ELT. It will provide a wide-field correction for the first-light instrument MICADO. The Low-Order wavefront modes will be sensed on 3 Natural Guide Stars with Shack-Hartmann Wavefront Sensors, so-called the LO WFS. In the presented work, we focus on the numerical study of the main aspects that depend on the LO WFS design and operational use: low-order sensing performance and sky coverage.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
C. Plantet, G. Agapito, C. Giordano, L. Busoni, M. Bonaglia, S. Esposito, C. Arcidiacono, F. Cortecchia, P. Ciliegi, E. Diolaiti, M. Bellazzini, R. Ragazzoni, and P. Feautrier "LO WFS of MAORY: performance and sky coverage assessment", Proc. SPIE 10703, Adaptive Optics Systems VI, 1070346 (12 July 2018); https://doi.org/10.1117/12.2313175
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Cited by 3 scholarly publications.
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KEYWORDS
Sensors

Infrared radiation

Stars

Adaptive optics

Error analysis

Tomography

Computer simulations

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