论文标题
Mavis：自适应光学模块的性能估计
MAVIS: performance estimation of the adaptive optics module
论文作者
论文摘要
MCAO辅助可见成像仪和光谱仪（MAVIS）是ESO非常大型望远镜（VLT）的新仪器。 Its Adaptive Optics Module (AOM) must provide extreme adaptive optics correction level at low galactic latitude and high sky coverage at the galactic pole on the FoV of 30arcsec of its 4k x 4k optical imager and on its monolithic Integral Field Unit, thanks to 3 deformable mirrors (DM), 8 Laser Guide Stars (LGS), up to 3 Natural Guide Stars (NGS) and 11 Wave Front Sensors （WFS）。需要仔细的性能估算来推动该模块的设计并评估系统和子系统要求的实现。在这里，我们介绍了去年对此主题所做的工作：我们更新了系统参数，以说明B期设计和更现实的条件，并且我们从分析和端到端模拟中产生了一系列结果，这些结果应尽可能完整地了解系统的性能。
The MCAO Assisted Visible Imager and Spectrograph (MAVIS) is a new visible instrument for ESO Very Large Telescope (VLT). Its Adaptive Optics Module (AOM) must provide extreme adaptive optics correction level at low galactic latitude and high sky coverage at the galactic pole on the FoV of 30arcsec of its 4k x 4k optical imager and on its monolithic Integral Field Unit, thanks to 3 deformable mirrors (DM), 8 Laser Guide Stars (LGS), up to 3 Natural Guide Stars (NGS) and 11 Wave Front Sensors (WFS). A careful performance estimation is required to drive the design of this module and to assess the fulfillment of the system and subsystems requirements. Here we present the work done on this topic during the last year: we updated the system parameters to account for the phase B design and for more realistic conditions, and we produced a set of results from analytical and end-to-end simulations that should give a as complete as possible view on the performance of the system.
