Connecting galaxy evolution and the growth of supermassive black holes

该项目将专注于确定活动星系核(AGN)，并将它们的性质与它们所在星系的演化联系起来。我们将使用星系调查，结合来自一系列设施的数据来识别处于不同宇宙纪元和不同演化状态的星系。然后，我们将使用多波长数据集、红外成像和无线电数据来识别这些星系中的活动星系核，并确定它们的性质。我们将跟踪活动星系核活动的水平如何依赖于星系的性质，以提供新的洞察，以促进和调节整个演化中的星系群体中黑洞的增长。

This project will focus on identifying Active Galactic Nuclei (AGN) and connecting their properties with the evolution of the galaxies they lie in. We will use galaxy surveys, incorporating data from a range of facilities to identify galaxies at different cosmic epochs and in different evolutionary states. We will then use multiwavelength datasets, infrared imaging, and radio data to identify AGN within these galaxies and determine their properties. We will track how the levels of AGN activity depend on the galaxy properties to provide new insights into the processes fuelling and regulating black hole growth across the evolving galaxy population.