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Further developments following the recent PanEx paper would focus on creating a new AME model. We have been discussing that this model should not rely on Commander templates as for a1 and a2—neither from Planck nor BeyondPlanck—and that it would be better to model AME using FIR dust emission. Additionally, injecting small scales by following a similar approach to the s5 and d10 models, and also the new f2 one (currently in development) would be highly valuable. Producing maps at nside = 2048, 4096, and 8192 would also be beneficial.
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