Unveiling the role of environment on the growth of galaxies and dark-matter halos

星系与周围的气体有着复杂的关系。宇宙网细丝对晕和星系的生长起着特别重要的作用：模拟表明，宇宙中大约40%的暗物质存在于细丝中，它们充当着将暗物质和中性冷气体送入晕和星系的管道。中性冷气体一旦吸积到星系上，几乎总是会形成恒星，在这一点上，它很容易通过星光检测到。然而，尽管我们是星系形成和成长的关键角色，但我们对宇宙网的气体成分知之甚少，直到它到达星系附近。在这个项目中，你将把遥远类星体光谱中的过量吸收与通过星系位置检测到的细丝交叉关联，以了解远离暗物质晕影响的宇宙网的气体含量。你将使用eBOSS和DESI数据，它们一起提供了穿透低红移宇宙网的视线的dennial样本。你的观测工作将得到宇宙流体动力学模拟工作的补充

Galaxies have a complex relationship with surrounding gas. Cosmic-web filaments take on especially important roles for halo and galaxy growth: simulations indicate that around 40 percent of the Dark Matter in the Universe is found within filaments, and they act as conduits that feed Dark Matter and neutral, cold gas into halos and galaxies. The neutral cold gas, once accreted onto a galaxy, will almost always form stars, at which point it becomes easily detectable via starlight. However, although a key player in the formation and growth of galaxies, we know astoundingly little about the gas component of the cosmic web, before it reaches the vicinity of a galaxy.In this project, you will cross-correlate excess absorption in the spectra of distant quasars with filaments detected via the positions of galaxies, to understand the gas content of the cosmic web, far from the influence of dark matter halos. You will work with eBOSS and DESI data, which together provide the densest sample of lines of sight that pierce the low-redshift cosmic web. Your observational work will be complemented by work in cosmological hydrodynamical simulations