The simulation of the optical turbulence (OT) for astronomical applications obtained with non-hydrostatic atmospherical models at meso-scale presents, with respect to measurements, some advantages. The future of the ground-based astronomy relies upon the potentialities and feasibility of the ELTs. Our ability in knowing, controlling and 'managing' the effects of the turbulence on such a new generation telescopes and facilities are determinant to assure their competitiveness with respect to the space astronomy. In the past several studies have been carried out proving the feasibility of the simulation of realistic Cn2 profiles above astronomical sites. The European Community (FP6 Program) decided recently to fund a Project aiming, from one side, to prove the feasibility of the OT forecasts and the ability of meso-scale models in discriminating astronomical sites from optical turbulence point of view and, from the other side, to boost the development of this discipline at the borderline between the astrophysics and the meteorology. In this contribution I will present the scientific and technological goals of this project, the challenges for the ground-based astronomy that are related to the success of such a project and the international synergies that have been joint to optimize the results.
The automation of optical transient discovery and classification in Rubin-era time-domain astronomy
Northwestern University（西北大学）；Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA)（天体物理学跨学科探索与研究中心）；University of Minnesota（明尼苏达大学）；California Institute of Technology（加州理工学院）
nmma: An extended Bayesian framework for Nuclear Multimessenger Astronomy in the Era of Next-Generation Detectors
Universität Potsdam（波茨坦大学）；Universiteit Utrecht（乌得勒支大学）；Nikhef（尼赫夫国家粒子物理研究所）；University of Ferrara（费拉拉大学）；INFN, Sezione di Ferrara（意大利国家核物理学院费拉拉分部）；INAF, Osservatorio Astronomico d’Abruzzo（意大利国家天体物理研究所阿布鲁佐天文台）；U. Minnesota（明尼苏达大学）；Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut)（马克斯·普朗克引力物理研究所（爱因斯坦研究所））
Towards the forecast of atmospheric parameters and optical turbulence above an astronomical site on 24h time scale
大气参数和光学湍流预报在地基天文中的应用是非常关键的，主要是队列调度。到目前为止，大多数努力已经解决了我们的小组在开发算法的光学湍流（CN 2）和所附的综合天体气候参数和量化的性能的Astro-Meso-Nh包在重建这些参数。此外，还对Meso-Nh在重建地基天文学相关大气参数方面的性能进行了深入的分析。我们的研究总是提到夜间制度。为了将我们的研究应用到白天的时间制度，我们提出，在这方面的贡献，通过比较模型输出和测量的经典大气参数相关的地基天文学在夜间和白天的时间得到的初步结果。我们选择了Roque de los Muchachos天文台（加那利群岛）作为测试案例，该天文台提供了由同一峰会/天文台上不同望远镜的不同传感器提供的非常扩展的测量集。接近地面的典型的白天的对流制度是非常不同的稳定制度的特点夜间。因此，这项研究的目的是扩大域的Astro-Meso-Nh代码的有效性，以新的湍流制度，它允许覆盖一天的24小时。这种方法不仅可以应用于太阳望远镜（例如EST），而且可以应用于范围更广的科学领域，而不仅仅是在卫星通信等天文学方面。
Establishing baseline model performances for optical turbulence forecasting
INAF Osservatorio Astrofisico di Arcetri（意大利国家天体物理研究所阿切尔西天文台）；ADONI: ADaptive Optics National laboratory of INAF（意大利国家天体物理研究所自适应光学国家实验室）；Large Binocular Telescope（大型双筒望远镜）
European Southern Observatory（欧洲南方天文台）；Institute of Physics, École Polytechnique Fédérale de Lausanne (EPFL)（洛桑联邦理工学院物理研究所）；IRFU, CEA, Université Paris-Saclay（法国原子能和替代能源署法国研究和技术核物理研究所巴黎萨克雷大学）；Department of Astronomy, Faculty of Mathematics, University of Belgrade（贝尔格莱德大学数学学院天文学系）；Hamburger Sternwarte, Universität Hamburg（汉堡大学天文台）；INAF OACN（意大利国家天体物理研究所卡塔尼亚天文台）；Astronomical Institute of Charles University（查理大学天文研究所）；Instituto de Astrofísica de Canarias（加那利群岛天体物理研究所）
Deep Investigation of Neutral Gas Origins (DINGO): Options for the Processing and Storage of Radio Astronomy Data for robust Deep Spectral Line Imaging in the SKA-Era using uv-Grids
International Centre for Radio Astronomy Research, University of Western Australia（西澳大利亚大学国际无线电天文研究中心）；Australian SKA Regional Centre (AusSRC), University of Western Australia（西澳大利亚大学澳大利亚SKA区域中心）；Pawsey Supercomputing Research Centre（珀西超级计算研究中心）；Oak Ridge National Laboratory（橡树岭国家实验室）；Australia Telescope National Facility, CSIRO Space & Astronomy（CSIRO空间与天文澳大利亚望远镜国家设施）；ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D)（ARC三维全天空天体物理学卓越中心）
The Role of Artificial Intelligence in the SKA Era
Centre for Artificial Intelligence, Zurich University of Applied Sciences ZHAW（苏黎世应用科学大学人工智能中心）；Institute of Business Information Technology, Zurich University of Applied Sciences ZHAW（苏黎世应用科学大学商业信息技术研究所）
PhoPS: An automated photometric pipeline for survey-era astronomy
Türkiye National Observatories, TUG（土耳其国家天文台）；The Scientific and Technological Research Council of Türkiye (TÜBİTAK)（土耳其科学技术研究委员会）；Instituto de Astrofísica de Andalucía (IAA-CSIC)（安达卢西亚天体物理研究所）；LIRA, CNRS UMR8254, Observatoire de Paris（巴黎天文台）
An agentic framework for gravitational-wave counterpart association in the multi-messenger era
Department of Astronomy, School of Physics（天文学系，物理系）；Kavli Institute for Astronomy and Astrophysics（天体物理研究所）；Institute for Gravitational Wave Astronomy（引力波天文研究所）；School of Information Science and Technology（信息科学与技术学院）；National Astronomical Observatories（国家天文台）
