The splashback radius of halos from particle dynamics: III. Halo catalogs, merger trees, and host-subhalo relations
Benedikt Diemer

TL;DR
This paper provides comprehensive halo catalogs, merger trees, and host-subhalo relations for multiple simulations, incorporating various halo boundary definitions including the splashback radius, to improve understanding of dark matter halo properties.
Contribution
It introduces new halo catalogs and merger trees with multiple boundary definitions, including splashback, and a novel data format for better analysis of halo structures.
Findings
Multiple halo boundary definitions compared and related.
Updated model for splashback and spherical overdensity connection.
Publicly available catalogs and tools for the community.
Abstract
Virtually any investigation involving dark matter halos relies on a definition of their radius, mass, and of whether they are a subhalo. The halo boundary is most commonly defined to include a spherical overdensity contrast (such as R200c, Rvir, and R200m), but different thresholds lead to significant differences in radius and mass. The splashback radius has recently been suggested as a more physically motivated (and generally larger) halo boundary, adding to the range of definitions. It is often difficult to assess the impact of a particular choice because most halo catalogs contain only one or a few definitions and generally only one set of host-subhalo relations. To alleviate this issue, we present halo catalogs and merger trees for 14 N-body simulations of LambdaCDM and self-similar universes. Based on ROCKSTAR catalogs, we compute additional halo properties using the SPARTA code…
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