The aox--HeII EW Connection in Radio-Loud Quasars

The catalog and research note presenting the X-ray and HeII EW properties of Radio-loud quasars. Our results indicate that the X-ray emission from typical RLQs largely originates in the corona and not from a jet-linked component.本星表与研究简报阐述了射电噪类星体（Radio-loud quasars）的X射线及HeⅡ等效宽度（Equivalent Width, EW）特性。本研究结果表明，典型射电噪类星体的X射线辐射主要源自黑洞冕，而非与喷流相关的成分。