The role of galaxy environment on the star forming intensity of high-redshift radio sources

在恒星形成最大的宇宙时代，射电源在其宿主星系中显示出广泛的恒星形成活动。我们的目的是验证恒星形成强度受射电源环境控制的假设。这对于理解开启（合并）和关闭（agn驱动的淬火）恒星形成的物理过程非常重要。利用赫歇尔和斯皮策太空望远镜，我们绘制了64个高红移射电星系和类星体的完整3CR样本

During the cosmic era of maximum star formation, radio sources show a broad range of star formation activity in their host galaxies. We aim to check the hypothesis that the star forming intensity is controlled by the environment of the radio sources. This is important for understanding the physical processes that turn star formation on (mergers) and off (AGN-driven quenching).Using the Herschel and Spitzer Space Telescopes, we have mapped the complete 3CR sample of 64 radio galaxies and quasars at high redshift (1