Extended Data Fig. 1: The field of view of the MIRI/MRS instrument relative to the size of the central galaxy in the Phoenix Cluster. | Nature

Extended Data Fig. 1: The field of view of the MIRI/MRS instrument relative to the size of the central galaxy in the Phoenix Cluster.

From: Directly imaging the cooling flow in the Phoenix cluster

Extended Data Fig. 1

The field of view of each of the four MIRI channels shown over a 3-color image of the core of the Phoenix cluster using data from HST/ACS in the F475W, F775W, and F850LP filters. The dust-obscured AGN lies at the center of the brightest cluster galaxy. The angular and physical scales are annotated in the bottom-left.

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