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Dianoga LR set

  • Authors: Ragone-Figueroa et al.
  • Contact: cinthia.ragone@unc.edu.ar
  • Pub-Date: 2018
  • Last modification: 2018


24 zoomed-in regions of massive galaxy clusters selected from a parent gravity only simulation of a 1$h^{−1}$ Gpc box. The regions surround all the 24 haloes with final $M_{200} > 8 \times 10^{14} h^{−1} M_{\odot}$. Each region was re-simulated at higher resolution including state-of-the-art baryonic physics. The set also includes 5 less massive clusters (D2, D3, D4, D5 and D9) with $M_{200} \sim 1 \times 10^{14} h^{−1} M_{\odot}$. The mass resolution for the DM and gas particles is $m_{DM} = 8.47\times 10^8 h^{−1} M_{\odot}$ and $m_{gas} = 1.53 \times 10^8 h^{−1} M_{\odot}$, respectively. More information in the reference paper.


Snapshots and subfind files for the 29 runs can be found in IATE storage at /mnt/simulations/dianoga_LR


Simulations set presented in https://ui.adsabs.harvard.edu/abs/2018MNRAS.479.1125R/abstract


Python library to read snapshots and subfind files can be downloaded from https://github.com/aragagnin/g3read

wiki/catalogo_simulaciones/dianoga_lr_set.txt · Última modificación: 2022/07/08 23:39 por srgualpa