Pulsed UV lasers can provide useful "testbeams" for observatories that use optical detectors, especially fluorescence detectors, to measure high energy cosmic-rays. The light observed by the detector is proportional to the energy of the laser pulse. Since the absolute laser energy can be measured locally, a well-calibrated laser offers a practical way to test the photometric calibration of the cosmic-ray detector including atmospheric corrections. This poster will describe a robotic system for laser polarization and energy calibration. Laboratory measurements of laser energies and polarizations by energy probes from different manufactures will be presented
Analysis of Laser-Satellite Deconfliction for Astronomical Observatories
Institute for Astronomy, University of Hawaii at Manoa（夏威夷大学马诺阿分校天文研究所）；California Institute of Technology（加州理工学院）；Subaru Telescope, National Astronomical Observatory of Japan（日本国立天文台昴星团望远镜）；W. M. Keck Observatory（W.M.凯克天文台）
Demonstration of a Single-Laser-Diode-Pumped Ti:Sapphire Astrocomb on the Southern African Large Telescope
Heriot-Watt University（赫瑞-瓦特大学）；Max Planck Institute for the Science of Light（马克斯·普朗克光科学研究所）；Alexandria University（亚历山大大学）；Friedrich-Alexander-Universität Erlangen-Nürnberg（埃尔朗根-纽伦堡大学）；LASEROPTIK GmbH（LASEROPTIK有限公司）；South African Astronomical Observatory（南非天文台）；University of York（约克大学）
Demonstration of Time Delay Interferometry and Spacecraft Ranging in a Space-based Gravitational Wave Detector using the UF-LISA Interferometry Simulator
Thermal Deformation Reduction in High-Power Interferometry with Higher-Order Laser Modes
Université Paris Cité, CNRS, Astroparticule et Cosmologie（巴黎西岱大学，法国国家科学研究中心，粒子与宇宙学）；University of Florida（佛罗里达大学）；Institute for Gravitational Wave Astronomy, Henan Academy of Sciences（河南省科学院引力波天文研究所）；School of Physics and Astronomy, Beijing Normal University（北京师范大学物理与天文学院）；Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University（北京师范大学天文与前沿科学研究院）
