The codes allow to calculate various subhalo properties efficiently using semi-analytical models for wold dark matter (WDM). The results are well in agreement with those from numerical N-body simulations.
If you use the SASHIMI script to write a paper, please cite:
- A. Dekker, S. Ando, C.A. Correa and K.C.Y. Ng, arXiv: 2111.13137
- N. Hiroshima, S. Ando and T. Ishiyama, arXiv: 1803.07691
- A.D. Ludlow, S. Bose, R.E. Angulo, L. Wang, W.A. Hellwing, J.F. Navarro, S. Cole and C.S. Frenk, arXiv: 1601.02624