Adrian Price-Whelan
Adrian Price-Whelan
https://ui.adsabs.harvard.edu/abs/2017MNRAS.465...76M/abstract
Like the `NFWPotential`, instead of specifying mass, it could be useful to specify circular velocity and scale radius.
When working on #280, I fixed some bugs with running `fit_toy_potential()` with a log true potential. We should test this method with all relevant potential classes.
Right now, many of the potential classes have scale radii with different names (a, c, r_s, etc.). We could make them all consistent!
- [ ] Using MN3 potential to approximate an exponential density distribution in a galaxy model - [ ] Estimating radial and vertical periods of a collection of orbits from...
- [x] Add interface to Agama or Galpy Stäckel fudge - #280 - [ ] Add interface for other Agama action solvers - [ ] Add 1D action solver -...
e.g., `t=0` to be passed into `.energy()` or `.density()`
### Describe your changes Uses linear interpolation to interpolate a set of SCF coefficients over time. ### Checklist * [ ] Did you add tests? * [ ] Did you...
Metadata should include things like the type of integrator used to compute the orbit, etc.