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This data includes the key snapshots of the simulations in GADGAET-2 format. The folders, namely D0, D1, D2, and D3, correspond to the four galaxy models used in this study. The snapshots are printed from time=0 Gyr to 10Gyr in a timestep of 1 Gyr.
Computational methods, Galaxy Dynamics, Dark matter halo
Computational methods, Galaxy Dynamics, Dark matter halo
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
| views | 7 | |
| downloads | 1 |

Views provided by UsageCounts
Downloads provided by UsageCounts