Major mergers going Notts: challenges for modern halo finders

Behroozi, Peter; Knebe, Alexander; Pearce, Frazer R.; Elahi, Pascal; Han, Jiaxin; Lux, Hanni; Mao, Yao-Yuan; Muldrew, Stuart I.; Potter, Doug; Srisawat, Chaichalit

Abstract

Merging haloes with similar masses (i.e. major mergers) pose significant challenges for halo finders. We compare five halo-finding algorithms’ (ahf, hbt, rockstar, subfind, and velociraptor) recovery of halo properties for both isolated and cosmological major mergers. We find that halo positions and velocities are often robust, but mass biases exist for every technique. The algorithms also show strong disagreement in the prevalence and duration of major mergers, especially at high redshifts (z > 1). This raises significant uncertainties for theoretical models that require major mergers for, e.g. galaxy morphology changes, size changes, or black hole growth, as well as for finding Bullet Cluster analogues. All finders not using temporal information also show host halo and subhalo relationship swaps over successive timesteps, requiring careful merger tree construction to avoid problematic mass accretion histories. We suggest that future algorithms should combine phase-space and temporal information to avoid the issues presented.

Citation

Behroozi, P., Knebe, A., Pearce, F. R., Elahi, P., Han, J., Lux, H., Mao, Y.-Y., Muldrew, S. I., Potter, D., & Srisawat, C. (2015). Major mergers going Notts: challenges for modern halo finders. Monthly Notices of the Royal Astronomical Society, 454(3), https://doi.org/10.1093/mnras/stv2046

• Journal Article Type: Article
• Acceptance Date: Aug 31, 2015
• Publication Date: Oct 16, 2015
• Deposit Date: May 3, 2017
• Publicly Available Date: May 3, 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: 454
• Issue: 3
• DOI: https://doi.org/10.1093/mnras/stv2046
• Keywords: methods: numerical, galaxies: haloes, dark matter
• Public URL: https://nottingham-repository.worktribe.com/output/763600
• Publisher URL: https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stv2046
• Contract Date: May 3, 2017