RUI: Harnessing Rubin Observatory Data to Prepare Tomorrow's STEM Leaders: Galaxy Evolution and Large Scale Structure

银河系并不是均匀地分布在整个宇宙中。相反，它们被发现高度集中在称为集群的区域，并沿着连接集群的巨大细丝传播。这种大规模的结构被称为宇宙网。众所周知，大型、大质量的红色星系通常出现在密集的星系团中，避开了中间的细丝和稀疏的空隙。因此，星系的性质与它所处的环境有关。该项目支持的加州理工州立大学的本科生将使用鲁宾天文台的新数据来研究星系的属性，如颜色，大小，形状和方向，如何取决于它们的环境。星系性质与其宿主环境之间的相关性将有助于推断宇宙网如何以及何时形成，以及星系的演化是否取决于其环境。该项目将为来自STEM代表性不足群体的本科生提供有价值的研究培训。提议的团队将使用鲁宾天文台的光谱观测以及预览和早期光度数据来测试将星系团星系与其更广泛环境联系起来的各种形成和演化情景。具体来说，该团队将描述和比较星系团核心、外围和细丝中星系的特性。主要交付成果包括：（1）对已知超星系团细丝中的恒星形成星系进行有效的光谱跟踪，这将提供光度与光谱恒星年龄、颜色和红移的比较，还将为计算星系坠落时间提供可靠的运动学数据;（2）对最亮的星团星系（BCG）--丝状星系之间的排列进行测量，（3）测量星系在大尺度结构和星系团核心中的星族分布;（4）团簇内光（ICL）注入到团簇图像中以检验ICL恢复方法。星星的形成率和进入时间将被计算出来，并用于确定有多少星系通过丝状体进入可能有助于BCG和ICL的形成。ICL恢复方法将为研究ICL做好准备，一旦鲁宾天文台上线，深度图像可用。该奖项体现了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。

Galaxies are not found evenly distributed throughout the universe. Rather, they are found to be highly concentrated in regions called clusters and spread along vast filaments that connect the clusters. This large-scale structure is referred to as the cosmic web. It is known that large, massive, red galaxies are generally found in the dense clusters, avoiding the filaments and sparse voids in between. The properties of a galaxy are thus correlated with the environment in which it lives. Undergraduate students at California Polytechnic State University supported by this project will use new data from the Rubin Observatory to study how the properties of galaxies, such as color, size, shape, and orientation, depend on their environment. Correlations between the galaxy properties and their host environment will help deduce how and when the cosmic web formed, and whether the evolution of a galaxy depends on its environment. This project will provide valuable research training to undergraduate students from underrepresented groups in STEM. The proposing team will use spectroscopic observations as well as preview and early photometric data from the Rubin Observatory to test various formation and evolutionary scenarios that connect cluster galaxies to their broader environment. Specifically, the team will characterize and compare the properties of galaxies in cluster cores, outskirts and filaments. The main deliverables include: (1) Efficient spectral follow-up of star-forming galaxies in known supercluster filaments, which will provide a comparison of photometric versus spectroscopic stellar ages, colors and redshifts, and will also provide reliable kinematic data for calculating galaxy in-fall times; (2) A measurement of alignments between filament galaxies, the brightest cluster galaxy (BCG), and the filament itself in order to test the importance of galaxy in-fall along filaments into the cluster core; (3) The measurement of stellar populations of galaxies throughout the large-scale structures and cluster cores; and (4) The injection of intra-cluster light (ICL) into cluster images in order to test ICL recovery methods. Star formation rates and in-fall times will be calculated and used to determine how much galaxy in-fall through filaments can plausibly contribute to the buildup of the BCG and ICL. The ICL recovery methods will prepare the group for studying ICL once the Rubin Observatory comes online and deep images are available. The undergraduate students who perform the research will be recruited with inclusive intent and trained in technical methods alongside diversity, equity and inclusivity education.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.