UK ALMA Regional Centre Node 2020 - 2024

英国 ALMA 区域中心节点 2020 - 2024

• 批准号: ST/T001488/1
• 负责人: Gary Fuller
• 金额: $ 201.82万
• 依托单位: University of Manchester
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2020
• 资助国家: 英国
• 起止时间: 2020 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FT001488%2F1
• 关键词: UK; ALMA; Regional; Centre; Node

This proposal is for funding of the UK Node of the European ALMA Regional Centre, which will continue to provide the UK ALMA community with direct user support, training and specialized software for experiment design, scheduling, data analysis and astrophysical interpretation. The Atacama Large Millimetre Array (ALMA) is transformational, and is revolutionising astronomy in the millimetre and sub-millimetre band with angular resolution, sensitivity, imaging quality and spectral coverage orders of magnitude beyond what available only a few years ago. The range of scientific applications is very broad, stretching from comets to cosmology, but ALMA's key strength is the detailed imaging of the processes of star and planet formation in our own galaxy and in the Universe at large, directly addressing many of the key themes of STFC's astronomical vision. ALMA operates at a very dry high (5000m) site in the Atacama Desert of northern Chile, close to the edge of the radio atmospheric window. The telescope has been very successful in automating much of the data processing for standard modes of operation, producing acceptable images approaching publishable quality for astronomers who are not experts in interferometry. However, for full exploitation of science extraction from advanced imaging many users require and appreciate additional support from skilled interferometry experts. In addition, ALMA operations can at times be challenging, especially non-standard modes such as for ultra-high angular resolution imaging with physically extended telescope configurations in the shortest wavelength bands. The operating plan for ALMA devolves all user interaction and support to three regional centres (ARCs) in US, Japan and Europe. The European model is a distributed one, with a central coordinating Node based at ESO in Garching and all face-to-face user support and more advanced data analysis facilities and enhanced imaging provided by a network of individual Nodes funded at the national level. In addition to the ESO Node there a 7 regional Nodes across Europe with UK ALMA user support being provided by the UK Node housed at the University of Manchester. The UK Node provides user support tailored to the requirements of individual UK ALMA users to assist in maximising their scientific return on ALMA programmes. It also provides support to all UK ALMA users for the complete set of elements for their ALMA science programmes from proposal preparation through quality assurance assessment of their data (especially for those programmes involving non-standard operational modes), to advanced imaging and maximisation of science extraction. The Node also provides regular workshops to both enhance science extraction through advanced data processing/imaging, and ensures the distribution of information regarding new ALMA developments and capabilities. The UK Node also provides IT hardware (computing power and data storage) to simultaneously support several UK-led ALMA projects (through both face-to-face and remote support); including the hosting of large ALMA programmes and programmes for international consortia. The UK Node is involved in the development of new and enhanced software tools to assist UK ALMA users in their project planning and execution - for both new programmes and archival access projects. UK Node personnel participate in ALMA development and EOC (Extension and Optimisation of Capabilities) commissioning programmes to utilise existing UK Node skills to deliver such programmes, and in addition provide enhanced support for UK ALMA users with regard to new ALMA developments.The UK ALMA user community has benefitted from the expert support provided by the UK Node and has grown to be a major user of ALMA. In the last 3 years of ALMA operations (Cycles 4-6) successful UK ALMA users have been awarded 26% of all the approved European time.

该提案是为欧洲ALMA区域中心的英国节点提供资金，该节点将继续为英国ALMA社区提供直接的用户支持、培训和专门的实验设计、调度、数据分析和天体物理解释软件。阿塔卡马大型毫米阵列（ALMA）是革命性的，它正在毫米和亚毫米波段的天文学中掀起革命，其角度分辨率、灵敏度、成像质量和光谱覆盖范围比几年前要高几个数量级。科学应用的范围非常广泛，从彗星延伸到宇宙学，但ALMA的关键优势是对我们自己的星系和整个宇宙中恒星和行星形成过程的详细成像，直接解决STFC天文视野的许多关键主题。ALMA在智利北部阿塔卡马沙漠一个非常干燥的高海拔（5000米）地点工作，靠近无线电大气窗口的边缘。该望远镜在标准操作模式下的大部分数据处理自动化方面非常成功，为非干涉测量专家的天文学家提供了可接受的接近可发表质量的图像。然而，为了充分利用先进成像的科学提取，许多用户需要并感谢熟练干涉测量专家的额外支持。此外，ALMA的操作有时也具有挑战性，特别是在非标准模式下，例如在最短波长波段内使用物理扩展的望远镜配置进行超高角分辨率成像。ALMA的运作计划将所有用户互动和支持下放到美国、日本和欧洲的三个区域中心。欧洲模式是分布式的，中央协调节点设在加兴的ESO，所有面对面的用户支持和更先进的数据分析设施，以及由国家一级资助的单个节点网络提供的增强成像。除了ESO节点外，欧洲还有7个区域节点，由位于曼彻斯特大学的英国节点提供英国ALMA用户支持。英国节点为英国ALMA用户提供量身定制的用户支持，以帮助最大限度地提高ALMA项目的科学回报。它还为所有英国ALMA用户提供支持，为他们的ALMA科学项目提供从提案准备到数据质量保证评估（特别是那些涉及非标准操作模式的项目），到先进成像和科学提取最大化的完整元素集。该节点还提供定期研讨会，通过先进的数据处理/成像增强科学提取，并确保有关新的ALMA发展和能力的信息分发。英国节点还提供IT硬件（计算能力和数据存储），以同时支持几个英国领导的ALMA项目（通过面对面和远程支持）；包括主办大型ALMA方案和国际财团方案。英国节点参与开发新的和增强的软件工具，以帮助英国ALMA用户进行项目规划和执行-包括新计划和档案访问项目。英国节点人员参与ALMA开发和EOC（能力扩展和优化）调试项目，利用现有的英国节点技能来交付此类项目，此外还为英国ALMA用户提供有关新ALMA开发的增强支持。英国ALMA用户社区受益于英国节点提供的专家支持，并已成长为ALMA的主要用户。在ALMA运行的最后3年（周期4-6）中，成功的英国ALMA用户获得了所有批准的欧洲时间的26%。

项目成果

Observing the very early stages of the formation of a circumbinary planetary system in SVS 13

在 SVS 13 中观察环绕双星系统形成的早期阶段

• DOI: 10.5194/epsc2022-1031
• 发表时间: 2022
• 作者: Anglada G

Continuity of accretion from clumps to Class 0 high-mass protostars in SDC335

• DOI: 10.1051/0004-6361/201936043
• 发表时间: 2020-12
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: A. Avison;G. Fuller;N. Peretto;A. Duarte-Cabral;A. Rosen;A. Traficante;J. Pineda;R. Güsten;N. Cunningham

An ALMA study of hub-filament systems - I. On the clump mass concentration within the most massive cores

轮毂-细丝系统的 ALMA 研究 - I. 关于最大质量核心内的团块质量集中

• DOI: 10.1093/mnras/stab2674
• 发表时间: 2021
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Anderson M

Polycyclic aromatic hydrocarbon excitation in nearby spiral galaxies

附近螺旋星系中的多环芳烃激发

• DOI: 10.1093/mnras/staa1589
• 发表时间: 2020-06
• 期刊: MNRAS
• 作者: Bendo G. J.;Lu Nanyao;Zijlstra A.
• 通讯作者: Zijlstra A.

Tracing Evolution in Massive Protostellar Objects (TEMPO) -- I: Fragmentation and emission properties of massive star-forming clumps in a luminosity limited ALMA sample

追踪大质量原恒星天体的演化（TEMPO）——I：光度有限的 ALMA 样本中大质量恒星形成团块的破碎和发射特性

• DOI: 10.48550/arxiv.2309.05772
• 发表时间: 2023
• 作者: Avison A