Linking Starlight to Dark Matter
The research team, which included studies led by Zachary Scofield and Hyungjin Joo at Yonsei University, used both strong and weak gravitational lensing to map the cluster's mass distribution. Strong lensing provided data on the central mass, while weak lensing revealed how matter is distributed across the outer regions. The analysis confirmed that XLSSC 122 is still undergoing a merger, with galaxies continuing to come together.
A key finding involves intracluster light, a faint glow produced by stars no longer bound to individual galaxies. Webb's observations represent the earliest known detection of this light. Near the cluster's center, the shape of the intracluster light closely matches the distribution of dark matter inferred from strong gravitational lensing.
"In this cluster, the intracluster light essentially traces the dark matter," Finner said. "That light tells us that the cluster is in a merging state."