Collaborative Research: New MCMC-enabled Bayesian Methods for Complex Data and Computer Models Applied in Astronomy

协作研究：用于天文学中应用的复杂数据和计算机模型的新的 MCMC 支持贝叶斯方法

• 批准号: 0907185
• 负责人: Xiao-Li Meng
• 金额: $ 37.84万
• 依托单位: Harvard University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2009
• 资助国家: 美国
• 起止时间: 2009-07-15 至 2013-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0907185&HistoricalAwards=false
• 关键词: Collaborative; Research; New; MCMC; enabled

This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).The California-Boston AstroStatistics Collaboration is developing a new model-based strategy for statistical inference that embeds computer models into multilevel models that explicitly account for complexities of both astronomical sources and the data generation mechanisms inherent in new high-tech telescopes. The resulting highly structured models must be fully utilized in order to learn about the underlying astronomical and physical processes. This strategy requires state-of-the-art scientific computation, advanced methods for statistical inference, and careful model checking procedures. The Collaboration has a track record using these methods to solve outstanding data-analytic problems in astronomy. In addition, the PIs (van Dyk, Meng, and Yu) have substantial research experience in developing the methods that the Collaboration will extend, employ, and publicize: inferential and efficient computational methods under highly-structured models that involve multiple levels of latent variables and incomplete data. Such models are ideally suited to account for the many physical and instrumental filters of the data generation mechanism in high-energy astrophysics. The five astronomers (Chiang, Connors, Kashyap, Kelly, and Siemiginowska) all have expertise on the instrumentation and science of high-energy and/or optical astronomy, and, all have collaborated with statisticians in efforts to develop appropriate methods to address scientific questions. The collaboration specifically aims to develop a mixture of parametrized and flexible multi-scale models that can be combined with complex computer-models to describe spectral, spatial, and timing data, either marginally or jointly. The models are developed in a fully Bayesian framework that allows us to incorporate external information, provide coherent estimates of uncertainty, and calibrate statistical comparisons of proposed underlying physical models. These methods require the Collaboration to develop new sophisticated statistical computing techniques for Monte Carlo exploration of complex and often multi-modal posterior distributions.In recent years, technological advances have dramatically increased the quality and quantity of data available to astronomers. Newly launched or soon-to-be launched space-based telescopes are tailored to data-collection challenges associated with specific scientific goals. These instruments provide massive new surveys resulting in new catalogs containing terabytes of data, high resolution spectrography and imaging across the electromagnetic spectrum, and incredibly detailed movies of dynamic and explosive processes in the solar atmosphere. The spectrum of new instruments is helping scientists make impressive strides in our understanding of the physical universe, but at the same time generating massive data analysis challenges for scientists who study the resulting data. The complexity of the instruments, the complexity of the astronomical sources, and the complexity of the scientific questions leads to many subtle inference problem that require sophisticated statistical tools. For example, data are partially missing, are subject to varying measurement errors, and are contaminated with irrelevant artifacts. Scientists wish to draw conclusions as to the physical environment and structure of the source, the processes and laws which govern the birth and death of planets, stars, and galaxies, and ultimately the structure and evolution of the universe. Sophisticated astrophysics-based computer-models are used along with complex mathematical models to predict the data observed from astronomical sources and populations of sources. The California-Boston AstroStatistics Collaboration aims to tackle outstanding statistical problems generated in astrophysics by establishing frameworks for the analysis of complex data using state-of-the-art statistical, astronomical, and computer models. In so doing the Collaboration will not only develop new methods for astronomy but will also use these problems as a spring board in the development of new general statistical methods, especially in signal processing, multilevel modeling, computer modeling, and computational statistics.

该奖项是根据2009年《美国复苏和再投资法案》(公法111-5)资助的。加州-波士顿天体统计合作正在开发一种新的基于模型的统计推断策略，将计算机模型嵌入到多层模型中，明确说明天文来源和新的高科技望远镜固有的数据生成机制的复杂性。必须充分利用由此产生的高度结构化的模型，以便了解基本的天文和物理过程。这一战略需要最先进的科学计算、先进的统计推断方法和仔细的模型检验程序。在使用这些方法解决天文学中悬而未决的数据分析问题方面，该合作有着良好的记录。此外，PI(van Dyk、Meng和Yu)在开发合作将扩展、采用和宣传的方法方面拥有丰富的研究经验：在涉及多级别潜在变量和不完整数据的高度结构化模型下的推理和高效计算方法。这类模型非常适合于解释高能天体物理学中数据生成机制的许多物理和仪器过滤器。这五位天文学家(Chiang、Connors、Kashyap、Kelly和Siemiginowska)都在高能和/或光学天文学的仪器和科学方面拥有专业知识，并且都与统计学家合作，努力开发适当的方法来解决科学问题。这项合作的具体目的是开发一种混合的参数化和灵活的多尺度模型，可以与复杂的计算机模型相结合，以边缘或联合的方式描述光谱、空间和时间数据。这些模型是在完全贝叶斯框架内开发的，允许我们纳入外部信息，提供对不确定性的一致估计，并校准拟议的基本物理模型的统计比较。这些方法需要合作开发新的尖端统计计算技术，用于蒙特卡罗探索复杂且往往是多模式的后验分布。近年来，技术进步显著提高了天文学家可用数据的质量和数量。新发射或即将发射的天基望远镜是为与具体科学目标相关的数据收集挑战量身定做的。这些仪器提供了大规模的新调查，产生了包含TB级数据的新目录，高分辨率光谱分析和电磁光谱成像，以及关于太阳大气中动态和爆炸过程的令人难以置信的详细电影。一系列新仪器正在帮助科学家在我们对物理宇宙的理解方面取得令人印象深刻的进展，但同时也给研究结果数据的科学家带来了大量数据分析的挑战。仪器的复杂性、天文来源的复杂性和科学问题的复杂性导致了许多微妙的推理问题，需要复杂的统计工具。例如，数据部分丢失，受到不同测量误差的影响，并被不相关的人工制品污染。科学家们希望得出关于源的物理环境和结构、支配行星、恒星和星系的诞生和死亡的过程和规律，以及最终宇宙的结构和演化的结论。复杂的基于天体物理学的计算机模型与复杂的数学模型一起被用来预测从天文来源和来源群体观察到的数据。加州-波士顿天体统计合作旨在通过建立使用最先进的统计、天文和计算机模型分析复杂数据的框架来解决天体物理学中产生的突出统计问题。通过这样做，合作不仅将为天文学开发新的方法，而且还将把这些问题作为开发新的通用统计方法的跳板，特别是在信号处理、多水平建模、计算机建模和计算统计方面。