ideas.md

• Kathryn: The disk mevement should manifest itself as a m=1 radialy-dependens in the expansion. Still need to separate from the wake?

• Nico: Can we test the amplitude of the "vibrations" in the MW using the BFE. See https://arxiv.org/abs/1902.03275

• Robyn S: Using streams to measure how the DM halo is chaning in time following Buist & Helmi see Figure 12.

• Adrian: Build a stellar halo to study the effect of substrucure along the lines of Bullock and Jhonston.

• Build a stellar halo to study the effect of the Wake on the stellar halo.

• Kathryn and more: Chracterize the DM potential from the LMC's DM Wake.

• Nico: Quantify Chaos in the combine potential?

• Nico: How axion variables look in the time-dependent potential?

• Chervin and others: Apply the BFE in Sgr and the LMC sims.

• Nico: Can we take one of the aquarius halos and add them a disk and an LMC? Using N-body sims?

• G: Eddie Illsutris Ids the BFE. Compare Illustris halos with ideal simulations. If the BFE expansion works with the Illustris Halos.

• G: Weak lensing talk To Eduardo R. about this. Lensing signal with the LMC. At what radius could weak lensing signals could be contaminating by the LMC.

• G: CMB anisotropy, any component from the LMC.