[5] That study made use of data from Cluster Lensing and Supernova survey with Hubble (CLASH) as well as other sources.

The temperature along with the entropy maps show cool, entropic gases trailing the subcluster in a southwesterly direction, which is consistent with core shredding.

The hot intracluster medium has an extension to the southeast along with a little indication of two cD galaxies located within the cluster.

The presence of (kT ≥ 15 keV) gas in the southeast portion of the cluster has been cited, reported, and confirmed by Chandra.

Overall background normalization was used to measure the ratio of the count rate of high energy frequences (which is known to be around 9-12 keV).