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-<markdown>
-# Dianoga LR set
-- Authors: Ragone-Figueroa et al.
-- Contact: cinthia.ragone@unc.edu.ar
-- Pub-Date: 2018
-- Last modification: 2018
-## Description
-</markdown>
-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
-<markdown>
-## 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
-</markdown>