WoU-MMA: Mapping the host galaxies of low-frequency gravitational-wave sources

引力波是爱因斯坦将引力描述为扭曲时空的基本预测。就像电磁波一样，引力波信号也有一个频谱，可以来自过多的信号源。虽然地球上的探测器已经从与太阳质量相似的黑洞合并中观测到引力波，但更大质量黑洞的合并仍然难以捉摸。然而，通过利用银河系中脉冲星的精确计时运动，我们离制造星系级探测器越来越近，这种探测器可以测量宇宙中最大的黑洞发出的引力波信号。这个研究小组将创建一个可能包含这种大质量黑洞对的星系目录。这将允许研究人员参考引力波搜索发现的可能的天空位置回到这个目录，并更精确地确定信号的起源。该项目将资助两名多信使科学研究生的培训。它将产生一个学生开发的网络工具，用于检查和过滤来自smbhb的引力波信号的候选宿主星系。这个网络工具将作为天体物理学研究人员纳米重力学生团队（STARS）计划的一个综合活动进行测试和改进。位于范德比尔特大学和加州大学伯克利分校的研究小组将为超大质量黑洞双星（SMBHB）系统的多信使发现开辟道路，并构建低频随机引力波（GW）背景的观测驱动模型。这项工作是基于两个大质量星系的目录，这些目录来自广域红外巡天探测器；一个目录是全天空的，但只完成到z0.45，另一个探测z1，但只部分覆盖天空。在加州大学伯克利分校，团队成员将开展一个增强和增强项目，为多信使研究提供关键数据，包括星系恒星质量和常驻超大质量黑洞质量。在范德比尔特大学，团队成员将在不久的将来进行脉冲星计时阵列运动中模拟单个smbhb的发现，然后过滤包含在GW统计定位区域内的潜在宿主星系。这将产生一组基于星系和gw推断的SMBHB属性的主机排序协议。在项目的最后阶段，整个团队将结合他们的专业知识，根据统计权重，用smbhb填充增强目录中的星系。他们将利用这些数据绘制gw天空图，研究集合背景信号角功率分布的各向异性，并探索其对近期信号探测前景的影响。该奖项旨在解决/推进宇宙之窗大构想的目标。该奖项反映了美国国家科学基金会的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。

Gravitational waves are a fundamental prediction of Einstein’s description of gravity as warped spacetime. Just like electromagnetic waves, there is a spectrum of gravitational-wave signals that can originate from a plethora of sources. While gravitational waves have been observed with Earth-based detectors from mergers of black holes similar in mass to the Sun, the mergers of more massive black holes remain elusive. However, by harnessing precision timing campaigns of pulsars in the Milky Way, we are getting closer to forging Galaxy-scale detectors that can measure gravitational-wave signals from the most massive black holes in the Universe. This research team will create a catalog of galaxies that might contain such pairs of massive black holes. This will allow researchers to reference likely sky-locations found by gravitational-wave searches back to this catalog and determine the origin of the signal much more precisely. This project will fund the training of two graduate students in multi-messenger science. It will result in a student-developed web-tool for the inspection and filtering of candidate host-galaxies of gravitational-wave signals from SMBHBs. This web-tool will be tested and improved as an integrated activity for the NANOGrav Student Teams of Astrophysics ResearcherS (STARS) program. Located at Vanderbilt University and UC Berkeley, the team will forge pathways to the multi-messenger discovery of supermassive black-hole binary (SMBHB) systems and construct observationally-driven models of the low-frequency stochastic gravitational wave (GW) background. This work is based on two massive-galaxy catalogs derived from the Wide-field Infrared Survey Explorer; one catalog is all-sky but only complete out to z0.45, the other probes z1 but with only partial sky coverage. At UC Berkeley, team members will conduct a program of augmentation and enhancement to provide crucial data for multi-messenger studies, including galaxy stellar masses and resident supermassive blackhole masses. At Vanderbilt, team members will conduct a realistic program of simulated discoveries of individual SMBHBs in near-future pulsar-timing array campaigns, followed by the filtering of potential host galaxies that are contained within the GW statistical localization regions. This will result in a set of host ranking protocols based on galaxy and GW-inferred SMBHB properties. In the project’s final stage, the full team will combine their expertise to populate galaxies in the enhanced catalogs with SMBHBs according to statistical weights. They will use these to make maps of the GW-sky, study the anisotropy of the ensemble background signal’s angular power distribution, and explore its effect on near-future signal detection prospects. This award addresses/advances the goals of the Windows on the Universe Big Idea.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.