28 June 2006 The laser guide star facility for Subaru Telescope
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Abstract
The purpose of this paper is to report on the current status of developing the new laser guide star (LGS) facility for the Subaru LGS adaptive optics (AO) system. Since two major R&D items, the 4W-class sum-frequency generating laser1 and the large-area-core photonic crystal fiber2, have been successfully cleared, we are almost ready to install the LGS facility to the Subaru Telescope. Also we report the result for LGS generation in Japan.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yutaka Hayano, Yutaka Hayano, Yoshihiko Saito, Yoshihiko Saito, Meguru Ito, Meguru Ito, Norihito Saito, Norihito Saito, Mayumi Kato, Mayumi Kato, Kazuyuki Akagawa, Kazuyuki Akagawa, Akira Takazawa, Akira Takazawa, Stephen A. Colley, Stephen A. Colley, Matthew C. Dinkins, Matthew C. Dinkins, Michael Eldred, Michael Eldred, Taras I. Golota, Taras I. Golota, Olivier Guyon, Olivier Guyon, Masayuki Hattori, Masayuki Hattori, Shin Oya, Shin Oya, Makoto Watanabe, Makoto Watanabe, Hideki Takami, Hideki Takami, Satoshi Wada, Satoshi Wada, Masanori Iye, Masanori Iye, } "The laser guide star facility for Subaru Telescope", Proc. SPIE 6272, Advances in Adaptive Optics II, 627247 (28 June 2006); doi: 10.1117/12.672583; https://doi.org/10.1117/12.672583
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