Space-based gravitational wave detectors based on the Laser Interferometer Space Antenna (LISA) design operate by synthesizing one or more interferometers from fringe velocity measurements generated by changes in the light travel time between three spacecraft in a special set of drag-free heliocentric orbits. These orbits determine the inclination of the synthesized interferometer with respect to the ecliptic plane. Once these spacecraft are placed in their orbits, the orientation of the interferometers at any future time is fixed by Kepler's Laws based on the initial orientation of the spacecraft constellation, which may be freely chosen. Over the course of a full solar orbit, the initial orientation determines a set of locations on the sky were the detector has greatest sensitivity to gravitational waves as well as a set of locations where nulls in the detector response fall. By artful choice of the initial orientation, we can choose to optimize or suppress the antennas sensitivity to sources whose location may be known in advance (e.g., the Galactic Center or globular clusters).
Numerical solutions for phase noise due to pointing jitter with the LISA telescope
激光干涉仪空间天线（LISA）的目的是通过航天器之间的长（2.5 Mkm）激光链路中的相位调制来探测引力波。要解决的其他噪声源包括由发射光束的可能角抖动引起的相位波动。本论文遵循我们的前一篇论文（Vinet et al 2019 Class.定量重力36，205 003）基于远场相位的分析研究。我们在这里解决的相位的数值处理，在发出的波前像差的第一顺序，但没有任何假设的静态偏置项。我们验证了，在相位变化，在静态错位的高阶项是一致的，我们在前面的文件中发现的结果。
Coupling of wavefront errors and pointing jitter in the LISA interferometer: misalignments of the interfering wavefronts
激光干涉仪空间天线是一种可预见的天基引力波探测器，其目标是在0.1 mHz至1 Hz的频率范围内探测10^20个应变。它是一个由三个航天器组成的三角形星座，边长为2.5 x 10^9米，每个航天器都有一对望远镜，可以同时发射和接收激光束，通过对接收到的波前与当地参考外差来测量星座臂。由于航天器和星座抖动，干扰（接收和本地）波前变得不对齐。我们研究分析失调和像差的干扰波前之间的耦合，并估计相关的外差信号的噪声的贡献。
Overlap reduction functions for a polarized stochastic gravitational-wave background in the Einstein Telescope-Cosmic Explorer and the LISA-Taiji networks
本文将基于球谐展开的重叠减少函数计算方法推广到第三代地基 Einstein Telescope-Cosmic Explorer 网络及 LISA-Taiji 空间联合任务，以分析极化随机引力波背景。
Demonstration of Time Delay Interferometry and Spacecraft Ranging in a Space-based Gravitational Wave Detector using the UF-LISA Interferometry Simulator
Subtraction of the confusion foreground and parameter uncertainty of resolvable galactic binaries on the networks of space-based gravitational-wave detectors
Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method
NASA Goddard Space Flight Center（美国宇航局戈达德太空飞行中心）；Artémis UMR 7250, Observatoire de la Côte d’Azur（蔚蓝海岸天文台阿尔特弥斯联合研究实验室）；Laboratoire Astroparticules et Cosmologie, Université Paris Diderot（巴黎第七大学亚原子物理与宇宙学实验室）
Constraints and detection capabilities of GW polarizations with space-based detectors in different TDI combinations
College of Physics, Chongqing University（重庆大学物理学院）；Department of Physics and Chongqing Key Laboratory for Strongly Coupled Physics, Chongqing University（重庆大学物理系及强耦合物理重庆市重点实验室）
Detection and characterization of instrumental transients in LISA Pathfinder and their projection to LISA
NASA Goddard Space Flight Center（美国宇航局戈达德太空飞行中心）；IRFU, CEA, Université Paris-Saclay（法国原子能与替代能源研究所，法国原子能委员会，巴黎萨克雷大学）；ARTEMIS, Observatoire de la Côte d’Azur（阿尔特米斯计划，蔚蓝海岸天文台）；SYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE（时间-频率和光学生物物理实验室，巴黎天文台，巴黎文理研究大学，法国国家科学研究中心，索邦大学，法国计量院）；Department of Physics, University of Trento（特伦托大学物理系）；Department of Physics, Aristotle University of Thessaloniki（塞萨洛尼基亚里士多德大学物理系）；Jet Propulsion Laboratory, California Institute of Technology（加州理工学院喷气推进实验室）
Impact of Spacecraft Orbit Uncertainties and Velocity Mismodeling on the LISA Gravitational-Wave Response
European Space Agency (ESA), European Space Research and Technology Centre (ESTEC)（欧洲空间局（ESA）欧洲空间研究与技术中心（ESTEC））；Leiden Observatory, Leiden University（莱顿天文台，莱顿大学）；Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)（马克斯·普朗克引力物理学研究所（爱因斯坦研究所））；Leibniz Universität Hannover, Institut für Gravitationsphysik（汉诺威莱布尼茨大学引力物理学研究所）；European Space Agency (ESA), European Space Operation Centre (ESOC)（欧洲空间局（ESA）欧洲空间运行中心（ESOC））
Accurate and efficient simulation-based inference for massive black-hole binaries with LISA
Universitá degli Studi di Milano-Bicocca（米兰比可卡大学）；INFN, Sezione di Milano-Bicocca（意大利国家核物理研究所米兰比可卡分部）；Max Planck Institute for Gravitational Physics (Albert Einstein Institute)（马克斯·普朗克引力物理学研究所（爱因斯坦研究所））；Nottingham Centre of Gravity & School of Mathematical Sciences, University of Nottingham（诺丁汉大学引力研究中心与数学科学学院）；Institute for Gravitational Wave Astronomy & School of Physics and Astronomy, University of Birmingham（伯明翰大学引力波天文学研究所与物理天文学院）
Mathematical derivation and verification of the amplitude of LISA's interferometric signals on an ultra-stable interferometer testbed
Max Planck Institute for Gravitational Physics (Albert Einstein Institute)（马克斯·普朗克引力物理研究所（爱因斯坦研究所））；Leibniz Universität Hannover（汉诺威莱布尼茨大学）；University of Granada（格拉纳达大学）
On the Effects of Pointing Jitter, Actuators Drift, Telescope Rolls and Broadband Detectors in Dark Hole Maintenance and Electric Field Order Reduction
