WOU-MMA: Improved Data Access for GW Astronomy

WOU-MMA：改进 GW 天文学的数据访问

• 批准号: 2011966
• 负责人: Jonah Kanner
• 金额: $ 39万
• 依托单位: California Institute of Technology
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2020
• 资助国家: 美国
• 起止时间: 2020-10-01 至 2023-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2011966&HistoricalAwards=false
• 关键词: WOU; MMA; Improved; Data; Access

This award supports research in relativity and relativistic astrophysics and it addresses the priority areas of NSF's "Windows on the Universe" Big Idea. Gravitational-wave astronomy is one of the most rapidly evolving fields in astrophysics. Over the past few years, the interferometer gravitational-wave observatories LIGO and Virgo have begun to record compact object mergers of black holes and neutron stars for the first time. These discoveries are having a tremendous impact on our ability to study the population of black holes in our universe, learn about fundamental particle physics through study of the dense interiors of neutron stars, test general relativity as never before, and investigate a range of other topics. Data from these cutting edge instruments are made available to the scientific community and the public through the Gravitational Wave Open Science Center (GWOSC) at gw-openscience.org. As LIGO and Virgo become more sensitive, the rate of discoveries is quickly accelerating. Starting in 2015, the number of observed compact object mergers has grown from 1, to 10, to 50. During the last observing run, LIGO and Virgo were observing mergers of black holes or neutron stars about once per week, and future upgrades are expected to make this rate grow. As we begin to record hundreds or thousands of these astrophysical events, the scientific community will need a new set of tools to access and analyze the information associated with these discoveries. This project will fund the construction of a new “event portal”, which will allow scientists, teachers, students, and enthusiasts around the world to browse catalogs of compact object mergers, study measurements of black hole properties, view graphics and plots, and listen to data converted to audio files, as well as download and analyze the associated interferometer data. The award also includes funding to host an Open Data Workshop to train students and scientists who wish to contribute to this new field of astronomy.Large collections of gravitational-wave events will invite a wide set of scientific investigations, but only if researchers with diverse interests are able to access and explore the associated data. Current structures on the GWOSC website provide only minimal support for derived data products (e.g., source parameters), and will not scale to hundreds of events. Going forward, the set of researchers interested in gravitational-wave science will likely broaden substantially to include more people interested in stellar populations, general relativity, nuclear astrophysics, and other fields. Many of these same people will be highly interested in derived data products, in addition to the gravitational-wave strain data GWOSC already hosts. Developing the event portal will enable these researchers to find and understand the data they need, and empower them to carry through their investigations. In addition, both the event portal and the Open Data Workshop will make gravitational-wave science more accessible to a wider array of researchers. Because less expertise will be needed to engage with this science, the event portal will “lower-the-bar” for entry into the field, and empower a more diverse group of scientists and students to benefit from GW observations.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

该奖项支持相对论和相对论天体物理学的研究，并解决了NSF“宇宙之窗”大理念的优先领域。引力波天文学是天体物理学中发展最快的领域之一。 在过去的几年里，干涉引力波天文台LIGO和Virgo已经开始首次记录黑洞和中子星的紧凑物体合并。 这些发现对我们研究宇宙中黑洞数量的能力产生了巨大的影响，通过研究中子星的致密内部来了解基本粒子物理学，以前所未有的方式测试广义相对论，并研究一系列其他主题。 来自这些尖端仪器的数据通过引力波开放科学中心（GWOSC）提供给科学界和公众，网址是gw-openscience.org。随着LIGO和Virgo变得越来越敏感，发现的速度正在迅速加快。 从2015年开始，观测到的紧凑型天体合并的数量从1个增加到10个，再增加到50个。 在上一次观测运行期间，LIGO和Virgo每周大约观测一次黑洞或中子星的合并，未来的升级预计会使这一速度增长。 当我们开始记录成百上千个这样的天体物理事件时，科学界将需要一套新的工具来访问和分析与这些发现相关的信息。 该项目将资助一个新的“事件门户”的建设，这将使世界各地的科学家，教师，学生和爱好者能够浏览紧凑物体合并的目录，研究黑洞属性的测量，查看图形和绘图，并收听转换为音频文件的数据，以及下载和分析相关的干涉仪数据。 该奖项还包括资助举办一个开放数据研讨会，以培训希望为这一新的天文学领域做出贡献的学生和科学家。大量的引力波事件将邀请广泛的科学调查，但前提是具有不同兴趣的研究人员能够访问和探索相关数据。GWOSC网站上的当前结构仅为派生数据产品提供最低限度的支持（例如，源参数），并且不会扩展到数百个事件。展望未来，对引力波科学感兴趣的研究人员可能会大幅扩大，包括更多对恒星种群、广义相对论、核天体物理学和其他领域感兴趣的人。除了GWOSC已经拥有的引力波应变数据外，这些人中的许多人将对衍生数据产品非常感兴趣。开发事件门户将使这些研究人员能够找到和了解他们所需要的数据，并使他们能够进行调查。 此外，活动门户和开放数据研讨会将使更广泛的研究人员更容易获得引力波科学。由于参与这一科学所需的专业知识较少，该活动门户网站将“降低进入该领域的门槛”，并使更多样化的科学家和学生群体能够从GW观测中受益。该奖项反映了NSF的法定使命，并通过使用基金会的智力价值和更广泛的影响审查标准进行评估，被认为值得支持。