Nick Koukoufilippas
Nick Koukoufilippas
@ccordoba12 just pinging you in case you might have missed it, seeing as this is the oldest issue that has no replies and no badges.
Tagging this as a v3 milestone since it's time we updated the old `halofit` option with a more modern version like the one implemented in `HMCode`.
Removed it from v3 milestones because it will work much better after #1063 .
No problem, I'll decouple it once we get to the v3 branch review. Note, this merely provides a framework for emulators to work, i.e. if a user wants they can...
Deleting stale branches won't affect the repo size, nor will it do (for the most part) if we only delete stuff from `HEAD`. The branches are merely pointers to specific...
**Potential solutions:** 1. Instead of only taking into account the n points at the edges for the n-th order extrapolation, we could try a `savgol_filter` or something similar near the...
**Sol. 1**: For example, here is what you can get using an extrapolation order of 2 on the Savitzky-Golay filtered prediction of the power spectrum with a window of 15....
Apart from the potential solutions I've listed I struggle to see anything obvious and computationally cheap that will solve the issue. Extrapolating accurately is difficult. Let me know if you...
**Update:** Sol1: Savgol filter, Sol2: best-fit, Sol3: use template. - Sol. 3 won't work as the slope of the template power spectra changes dramatically with different cosmologies. - Sol. 2...
yeah me too, I've already started doing that in my dev branches