Extended Data Fig. 3: A zoomed-in emission line spectrum of the central galaxy in the Phoenix Cluster.
From: Directly imaging the cooling flow in the Phoenix cluster
A subset of the MIRI channel 3 spectrum zoomed in on the [Ne vi] line. This spectrum includes only a single spaxel north of the nucleus. The formatting of everything is identical to Extended Data Fig. 2, except that there is no translucent orange region since this fit has not been bootstrapped. The two distinct kinematic components of the emission lines can be seen in purple.
