Cambridge Astronomical Survey Unit (CASU) (2023-2026): Powering Next Generation Survey Analysis and Processing

剑桥天文测量单位 (CASU)（2023-2026）：为下一代测量分析和处理提供动力

• 批准号: ST/X001857/1
• 负责人: Nicholas Walton
• 金额: $ 234.05万
• 依托单位: University of Cambridge
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2023
• 资助国家: 英国
• 起止时间: 2023 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FX001857%2F1
• 关键词: Cambridge; Astronomical; Survey; Unit; CASU

Observational survey astronomy is powering discovery, with the UK leading and benefiting from its investment, both financially and intellectually in state-of-the-art observational facilities. The last decade has seen the delivery of comprehensive imaging of both the northern and southern hemispheres in the near infrared using WFCAM and VISTA, with the UK leading these survey initiatives. These have and will provide key insights across a wide range of astrophysics. The next decade will witness the arrival of large scale spectroscopic surveys to probe in more detail key populations (be they galaxies, stars, asteroids) revealed by the imaging surveys. The UK is well poised to lead this scientific discovery, through involvement and definition of the specific surveys to be carried out on these facilities such as WEAVE, 4MOST and MOONS. The 2020s are beginning to fulfil its potential to be the decade of "total" survey astronomy enabling profound insights into astrophysics at all scales through the combination of comprehensive imaging and spectroscopic scale data. Ensuring the scientific potential of these facilities and surveys requires the availability of expertise and systems to optimally extract information from the data. Here the UK has a substantial lead with the Cambridge Astronomical Survey Unit (CASU) and its proven ability to provide cost effective data systems to the UK and wider communities. CASU have been at the forefront of survey astronomy, not only in pioneering techniques to optimally extract knowledge from survey data, but also in taking a proactive role in exploiting this information to produce world-leading research. This synergy and feedback between data processing and science delivery has been repeatedly demonstrated to be essential in ensuring delivery of the best possible science data products for exploitation by the widest community of UK and European astronomers. In the last decade, CASU generated science data products from VISTA, WFCAM and VST imaging and Gaia-ESO VLT spectroscopy have supported world-class research programmes across almost every UK institute involved in astrophysics. CASU are filling the astronomical data lake, the vital data resource which the community can mine, combine with other multi-wavelength data (e.g., Euclid, PLATO) and discover rare and unique objects for further detailed study by facilities such as the ELT or the JWST. The role of CASU is acknowledged in the wider context, with ESO relying on CASU to provide the science data products from its public surveys currently running on the ESO survey facilities: VISTA, the VST and its large spectroscopic surveys. CASU's provision to ESO will extend into the next decade supporting the delivery of the science data from ESO's new front line spectroscopic survey machine: 4MOST, and for the public survey programme envisaged for MOONS on the VLT. This grant proposal builds on the tremendous advances already made by CASU and requests funding for the period 2023-2026 for the following activities:- WP1: Design and development of the data management and analysis systems for the next generation of ESO / ING wide field massively multiplexed optical spectrographs WEAVE, MOONS and 4MOST;- WP2: Full operations of the WEAVE, MOONS and 4MOST pipelines, and responsibility of the delivery of the processed data products for release- WP3: Final maintenance, operation, post operation releases and user support of the science and analysis pipelines for the UK-led VISTA large scale surveys;- WP4: Deployment and operations of all CASU pipelines at the CASU-Data Processing Centre, itself hosted on the STFC IRIS Cloud Infrastructure In summary, support of the CASU programme ensures the UK pre-eminence in astronomical data analysis. CASU provides the high-quality science data products from significant UK investment in frontline spectroscopic facilities, vital in maximising the research impact for the UK astronomical community.

观测调查天文学正在为发现提供动力，英国在最先进的观测设施方面的投资在财政和智力上都处于领先地位并从中受益。在过去十年中，使用WFCAM和VISTA对北方和南半球进行了近红外全面成像，英国在这些调查活动中处于领先地位。这些已经并将提供广泛的天体物理学的关键见解。未来十年将见证大规模光谱调查的到来，以更详细地探测成像调查揭示的关键群体（无论是星系，恒星，小行星）。联合王国已做好充分准备，通过参与和确定将在WEAVE、4 MOST和MOONS等设施上进行的具体调查，领导这一科学发现。21世纪20年代开始发挥其潜力，成为“全面”巡天天文学的十年，通过综合成像和光谱尺度数据的结合，使人们能够深刻了解所有尺度的天体物理学。要确保这些设施和调查的科学潜力，就需要具备专门知识和系统，以便从数据中最佳地提取信息。在这方面，英国凭借剑桥天文测量单位（CASU）及其向英国和更广泛的社区提供成本效益高的数据系统的能力，处于实质性领先地位。CASU一直处于巡天天文学的最前沿，不仅在开拓技术，以最佳方式从巡天数据中提取知识，而且在利用这些信息进行世界领先的研究方面发挥积极作用。数据处理和科学交付之间的这种协同作用和反馈已多次被证明是必不可少的，以确保提供最好的科学数据产品，供英国和欧洲天文学家最广泛的社区利用。在过去的十年中，CASU从VISTA，WFCAM和VST成像以及Gaia-ESO VLT光谱学中产生的科学数据产品支持了几乎所有参与天体物理学的英国研究所的世界级研究计划。CASU正在填补天文数据湖，社区可以挖掘的重要数据资源，联合收割机与其他多波长数据（例如，欧几里得，柏拉图），并发现罕见和独特的对象，进一步详细研究的设施，如ELT或JWST。CASU的作用在更广泛的背景下得到了承认，ESO依靠CASU提供目前在ESO调查设施上运行的公共调查的科学数据产品：VISTA，VST及其大型光谱调查。CASU向ESO提供的服务将延续到下一个十年，以支持ESO新的前线光谱测量机器4 MOST提供科学数据，并支持为VLT上的MOONS设想的公共调查计划。该拨款提案建立在CASU已经取得的巨大进步的基础上，并要求在2023-2026年期间为以下活动提供资金：-WP 1：为下一代ESO / ING宽视场大规模多路复用光谱仪WEAVE，MOONS和4 MOST设计和开发数据管理和分析系统;-WP 2：WEAVE、MOONS和4 MOST管道的全面运行，以及交付经处理的数据产品以供发布的责任-WP 3：为英国领导的VISTA大规模调查提供科学和分析管道的最终维护、操作、操作后发布和用户支持;- WP 4：在CASU数据处理中心部署和运营所有CASU管道，该中心本身托管在STFC IRIS云基础设施上。总之，对CASU计划的支持确保了英国在天文数据分析方面的领先地位。CASU提供高质量的科学数据产品，来自英国对前线光谱设施的重大投资，这对最大限度地提高英国天文学界的研究影响至关重要。

项目成果

Multiwavelength detection of an ongoing FUOr-type outburst on a low-mass YSO

• DOI: 10.1093/mnrasl/slad201
• 发表时间: 2023-12
• 期刊: Monthly Notices of the Royal Astronomical Society: Letters
• 作者: Zhen Guo;‹. P. W. Lucas;R. Kurtev;J. Borissova;V. Elbakyan;C. Morris;A. Bayo;L. Smith;A. C. O. Garatti;C. Pe;D. Minniti;J. Jose;M. Ashraf;J. Alonso-Garc;N. Miller;H. Muthu;Hillenbrand Findeisen;C. Pe;Naylor Morrell

On the incidence of episodic accretion in Class I YSOs from VVV

• DOI: 10.1093/mnras/stad3780
• 发表时间: 2024-01
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: C. Contreras Peña-C.-Contreras Peña-2124046337;P. W. Lucas;Zhen Guo;L. Smith

Enlightening the Universe behind the Milky Way bulge I. Target selection of VVV bulge galaxies

启示银河系核球背后的宇宙 一、VVV核球星系的目标选择

• DOI: 10.1051/0004-6361/202347921
• 发表时间: 2024
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Duplancic F

The VST ATLAS quasar survey I: Catalogue of photometrically selected quasar candidates

VST ATLAS 类星体调查 I：光度选择的候选类星体目录

• DOI: 10.1093/mnras/stad516
• 发表时间: 2023
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Eltvedt A

High energy gamma-ray sources in the VVV survey -- II. The AGN counterparts

VVV 巡天中的高能伽马射线源——II。

• DOI: 10.48550/arxiv.2401.05542
• 发表时间: 2024
• 期刊: arXiv e-prints
• 作者: Donoso Laura G.