Possible trend in detector settling based on the previous filter used by MIRI. The mean and uncertainty in the slope of the first 30 minutes of the aperture extracted light curve is plotted for various Hot Rocks observations. Left plot shows previous imaging filters based on their central wavelength, the right plot includes the OPAQUE position for darks, the P750L prism for LRS and a coronagraphic filter. Observations which shared the same previous filters often display similar detector settling.