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We present a proper motion measurement for the halo globular cluster Pyxis, using HST/ACS data as the first epoch, and GeMS/GSAOI Adaptive Optics data as the second, separated by a baseline of ~ 5 yea...
2017SPIE EUV,X射线和伽玛射线天文学光学专题会议(Optics for EUV,X-Ray,and Gamma-Ray Astronomy VIII)。
2017SPIE天文光学专题会议(Astronomical Optics:Design,Manufacture,and Test of Space and Ground Systems)。
The goals of this work are to provide NIR polarimetry of the stellar sources in the central pc at the resolution of an 8m telescope for the first time, along with new insights into the nature of the k...
The Durham adaptive optics real-time controller was initially a proof of concept design for a generic adaptive optics control system. It has since been developed into a modern and powerful CPU based r...
Manufacturing of FRODOSpec red arm optics and mounts
Frida:the first instrument for the adaptive optics system of GTC
Testing the Optics of the instrument Elmer。
Adaptive Optics Observations of Active Galactic Nuclei:Zooming into the Central Parsec Region。
Guieloa:adaptive optics system for the 2.1-m spm unam Telescope。
Effect of scintillation on adaptive optics systems。
Wavefront outer scale measurements at San Pedro Mártir observatory. Its impact on adaptive optics performances。
Off-axis point spread function and efficiency for adaptive optics at San Pedro Mártir and other sites。

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