Understanding the effect of large-scale environment on DM halo structure and galaxy properties
Train Spherinator to reproduce 3D structure of DM in simulated galaxies
Select minimum number of output features based on minimum required accuracy of reconstruction (i.e. 5-10%)
Paint haloes in feature space using traditional interpretable halo properties (mass, concentration, spin, etc) to help interpret dominant features
Color points by large scale environment to find effect and produce predictions
Do the same for 3D baryon distribution (i.e. stars or gas)
Galaxy simulation parameter search: produce a robust metric for simulations to understand how close a given sub grid model gets to reproduce the properties of galaxies
Use Spherinator to represent stellar distributions of sims with minimum dimensionality (i.e. 2D or 3D)
Compare distribution of points of simulations and observations until a model is found that is statistically consistent
Model can then be used to deconstruct the physics of galaxy formation and to reconstruct histories of observed galaxies
Can also generate mocks on top of N-body sims
Detect outliers in simulations to test the input physics at the extremes of the distributions
Find compact representation of DM halo structure to provide robust models for Bayesian tests of CDM predictions regarding the haloes of observed galaxies
Use Spherinator to find minimum representation of entire sample of haloes in simulations with specific physics
Encoder network is then able to generate distributions that can be compared to mass models of galaxy kinematic data
Is the data consistent with the simulated distribution?
Eliminates the need to collapse diversity into mass, concentration axes
Allows to obtain the closest match of an observed RC in a simulation for consistency tests
Description of possible use cases for Spherinator
Understanding the effect of large-scale environment on DM halo structure and galaxy properties
Galaxy simulation parameter search: produce a robust metric for simulations to understand how close a given sub grid model gets to reproduce the properties of galaxies
Detect outliers in simulations to test the input physics at the extremes of the distributions
Find compact representation of DM halo structure to provide robust models for Bayesian tests of CDM predictions regarding the haloes of observed galaxies