092268

Radio-loud supermassive black holes (SMBHs) at the highest redshifts($zgtrsim6$) are some of the most intriguing targets for early Universe studiesas their radio properties may be the key to understanding early SMBH growth.Until recently however the known population of these objects was small butrecent targeted surveys have dramatically expanded this census. The X-rayproperties of these quasars are fundamentally important as they reveal both theoverall accretion processes in individual quasars and as a population the roleinverse Compton interactions with the CMB play in suppressing radio flux injets. We therefore propose a Fulfil Programme to complete the archive ofReionization-era radio-loud quasars. [truncated! Please see actual data for full text]

最高红移（$zgtrsim6$）的射电噪超大质量黑洞（SMBHs）是早期宇宙研究中最具吸引力的目标之一，其射电特性或许是理解早期超大质量黑洞生长机制的关键。然而，直到最近，这类天体的已知样本数量仍较为有限，而近期的针对性巡天已显著扩充了这一统计样本库。这些类星体的X射线特性至关重要：它们既揭示了单个类星体的整体吸积过程，也作为群体层面揭示了逆康普顿相互作用与宇宙微波背景（CMB）在抑制喷流射电流量中所扮演的角色。因此，我们提议开展一项Fulfil计划，以完善再电离时代射电噪类星体的档案库。[内容截断！请查阅实际数据获取完整文本]