Poster + Paper
29 August 2022 Final design of the GTC laser guide star wavefront sensor
Author Affiliations +
Conference Poster
Abstract
The Laser Guide Star Facility (LGSF) of GTC will generate a laser guide star (LGS) in the high atmosphere for the GTC Adaptive Optics System (GTCAO) to measure and correct the effect of the atmospheric turbulence. The GTCAO LGS Wavefront Sensor (LWS) will be based on a Shack Hartmann WFS and placed on the GTCAO optical bench, where the Natural Guide Star (NGS) Wavefront Sensor is already installed. The science dichroic splits the light beam so that the visible range (0.47-0.9μm) is reflected to the NGS WFS, and the infrared range 0.9-2.5μm is transmitted to the science instrument. A new second dichroic (LWS DC) will be installed in the visible path, to reflect 589nm (FWHM 12nm) towards the LWS, and to transmit the rest of the visible light to the NGS WFS. In addition, the system will count on an LGS calibration source. The proceeding describes the opto-mechanical design of the LWS System, covering its different subsystems: LWS Dichroic, LWS Sensor and LWS Calibration Unit.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. Simoes, M. Puga, M. Reyes García-Talavera, J. Patrón, O. Tubío, I. Montilla, F. Tenegi, J. Sánchez-Capuchino, and Víctor J. S. Béjar "Final design of the GTC laser guide star wavefront sensor", Proc. SPIE 12185, Adaptive Optics Systems VIII, 1218543 (29 August 2022); https://doi.org/10.1117/12.2629289
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KEYWORDS
Cameras

Wavefront sensors

Sodium

Calibration

Laser guide stars

Tolerancing

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