Santiago Avila
Sussing merger trees: the influence of the halo finder
Avila, Santiago; Knebe, Alexander; Pearce, Frazer R.; Schneider, Aurel; Srisawat, Chaichalit; Thomas, Peter A.; Behroozi, Peter; Elahi, Pascal J.; Han, Jiaxin; Mao, Yao-Yuan; Onions, Julian; Rodriguez-Gomez, Vicente; Tweed, Dylan
Authors
Alexander Knebe
Frazer R. Pearce
Aurel Schneider
Chaichalit Srisawat
Peter A. Thomas
Peter Behroozi
Pascal J. Elahi
Jiaxin Han
Yao-Yuan Mao
Julian Onions
Vicente Rodriguez-Gomez
Dylan Tweed
Abstract
Merger tree codes are routinely used to follow the growth and merger of dark matter haloes in simulations of cosmic structure formation. Whereas in Srisawat et. al. we compared the trees built using a wide variety of such codes, here we study the influence of the underlying halo catalogue upon the resulting trees. We observe that the specifics of halo finding itself greatly influences the constructed merger trees.We find that the choices made to define the halo mass are of prime importance. For instance, amongst many potential options different finders select self-bound objects or spherical regions of defined overdensity, decide whether or not to include substructures within the mass returned and vary in their initial particle selection. The impact of these decisions is seen in tree length (the period of time a particularly halo can be traced back through the simulation), branching ratio (essentially the merger rate of subhaloes) and mass evolution. We therefore conclude that the choice of the underlying halo finder is more relevant to the process of building merger trees than the tree builder itself. We also report on some built-in features of specific merger tree codes that (sometimes) help to improve the quality of the merger trees produced.
Citation
Avila, S., Knebe, A., Pearce, F. R., Schneider, A., Srisawat, C., Thomas, P. A., …Tweed, D. (2014). Sussing merger trees: the influence of the halo finder. Monthly Notices of the Royal Astronomical Society, 441(4), https://doi.org/10.1093/mnras/stu799
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 20, 2014 |
Online Publication Date | May 31, 2014 |
Publication Date | Jul 11, 2014 |
Deposit Date | May 9, 2017 |
Publicly Available Date | May 9, 2017 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 441 |
Issue | 4 |
DOI | https://doi.org/10.1093/mnras/stu799 |
Keywords | methods: numerical, galaxies: evolution, galaxies: haloes, dark matter |
Public URL | https://nottingham-repository.worktribe.com/output/732706 |
Publisher URL | https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stu799 |
Contract Date | May 9, 2017 |
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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf
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