GRAVITATIONALLY CONSISTENT HALO CATALOGS AND MERGER TREES FOR PRECISION COSMOLOGY

被引:492
作者
Behroozi, Peter S. [1 ,2 ]
Wechsler, Risa H. [1 ,2 ]
Wu, Hao-Yi [1 ,2 ]
Busha, Michael T. [3 ]
Klypin, Anatoly A. [4 ]
Primack, Joel R. [5 ]
机构
[1] Stanford Univ, Dept Phys, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
[2] SLAC Natl Accelerator Lab, Dept Particle Phys & Astrophys, Stanford, CA 94305 USA
[3] Univ Zurich, Inst Theoret Phys, CH-8006 Zurich, Switzerland
[4] New Mexico State Univ, Dept Astron, Las Cruces, NM 88003 USA
[5] Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA
基金
美国国家科学基金会;
关键词
dark matter; galaxies: abundances; galaxies: evolution; methods: numerical; DARK-MATTER HALOES; N-BODY SIMULATIONS; GALAXY FORMATION; MASS ACCRETION; STATISTICAL PROPERTIES; CLUSTER; EVOLUTION; HISTORY; MODEL; RATES;
D O I
10.1088/0004-637X/763/1/18
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a new algorithm for generating merger trees and halo catalogs which explicitly ensures consistency of halo properties (mass, position, and velocity) across time steps. Our algorithm has demonstrated the ability to improve both the completeness (through detecting and inserting otherwise missing halos) and purity (through detecting and removing spurious objects) of both merger trees and halo catalogs. In addition, our method is able to robustly measure the self-consistency of halo finders; it is the first to directly measure the uncertainties in halo positions, halo velocities, and the halo mass function for a given halo finder based on consistency between snapshots in cosmological simulations. We use this algorithm to generate merger trees for two large simulations (Bolshoi and Consuelo) and evaluate two halo finders (ROCKSTAR and BDM). We find that both the ROCKSTAR and BDM halo finders track halos extremely well; in both, the number of halos which do not have physically consistent progenitors is at the 1%-2% level across all halo masses. Our code is publicly available at http://code.google.com/p/consistent-trees. Our trees and catalogs are publicly available at http://hipacc.ucsc.edu/Bolshoi/.
引用
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页数:15
相关论文
共 53 条
[1]   The shape of dark matter haloes: dependence on mass, redshift, radius and formation [J].
Allgood, B ;
Flores, RA ;
Primack, JR ;
Kravtsov, AV ;
Wechsler, RH ;
Faltenbacher, A ;
Bullock, JS .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 367 (04) :1781-1796
[2]  
Allgood B. A, 2005, THESIS U CALIFORNIA
[3]  
[Anonymous], ASTROPH9712217 INSPI
[4]  
Behroozi P. S., 2012, ARXIV12076105
[5]   THE ROCKSTAR PHASE-SPACE TEMPORAL HALO FINDER AND THE VELOCITY OFFSETS OF CLUSTER CORES [J].
Behroozi, Peter S. ;
Wechsler, Risa H. ;
Wu, Hao-Yi .
ASTROPHYSICAL JOURNAL, 2013, 762 (02)
[6]  
Benson A. J., 2011, MNRAS, V419, P3590
[7]   Resolving cosmic structure formation with the Millennium-II Simulation [J].
Boylan-Kolchin, Michael ;
Springel, Volker ;
White, Simon D. M. ;
Jenkins, Adrian ;
Lemson, Gerard .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 398 (03) :1150-1164
[8]   Statistical properties of X-ray clusters: Analytic and numerical comparisons [J].
Bryan, GL ;
Norman, ML .
ASTROPHYSICAL JOURNAL, 1998, 495 (01) :80-99
[9]  
Cole S, 2008, MON NOT R ASTRON SOC, V383, P546, DOI [10.1111/j.1365-2966.2007.12516.x, 10.1111/j.1365-2966.2007.125l6.x]
[10]   Modeling luminosity-dependent galaxy clustering through cosmic time [J].
Conroy, Charlie ;
Wechsler, Risa H. ;
Kravtsov, Andrey V. .
ASTROPHYSICAL JOURNAL, 2006, 647 (01) :201-214