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# Dianoga LR set - Authors: Ragone-Figueroa et al. - Contact: cinthia.ragone@unc.edu.ar - Pub-Date: 2018 - Last modification: 2018 # Dianoga LR set - Authors: Ragone-Figueroa et al.- Contact: cinthia.ragone@unc.edu.ar- Pub-Date: 2018- Last modification: 2018
## Description 24 zoomed-in regions of massive galaxy clusters selected from a parent gravity only simulation of a 1h−1 Gpc box. The regions surround all the 24 haloes with final M200>8×1014h−1M⊙. 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 M200∼1×1014h−1M⊙. The mass resolution for the DM and gas particles is mDM=8.47×108h−1M⊙ and mgas=1.53×108h−1M⊙, 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
## Reference Simulations set presented in https://ui.adsabs.harvard.edu/abs/2018MNRAS.479.1125R/abstract ## Tutorial Python library to read snapshots and subfind files can be downloaded from https://github.com/aragagnin/g3read