期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 484, 期 3, 页码 3818-3830出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz278
关键词
methods: numerical; cosmological parameters; large-scale structure of Universe
资金
- LabEx OCEVU [ANR-11-LABX-0060]
- Action Incitative of Aix-Marseille Universite
- MUIR PRIN 2015 'Cosmology and Fundamental Physics: illuminating the Dark Universe with Euclid'
- Agenzia Spaziale Italiana [ASI/INAF/I/023/12/0]
- ASI [2016-24-H.0]
- INFN project 'INDARK'
A new fully non-linear reconstruction algorithm for the accurate recovery of the baryonic acoustic oscillations (BAO) scale in two-point correlation functions is proposed, based on the least action principle and extending the Fast Action Minimisation method by Nusser & Branchini (2000). Especially designed for massive spectroscopic surveys, it is tested on dark matter halo catalogues extracted from the DEUS-FUR Lambda cold dark matter simulation (Reverdy et al. 2015) to trace the trajectories of up to similar to 207000 haloes backward in time, well beyond the first-order Lagrangian approximation. The new algorithm successfully recovers the BAO feature in real and redshift space in both the monopole and the anisotropic two-point correlation function, also for anomalous samples showing misplaced or absent signature of BAO. In redshift space, the non-linear displacement parameter Sigma(NL) is reduced from 11.8 +/- 0.3 h(-1) Mpc at redshift z = 0 to 4.0 +/- 0.5 h(-1) Mpc at z similar or equal to 37 after reconstruction. A comparison with the first-order Lagrangian reconstruction is presented, showing that these techniques outperform the linear approximation in recovering an unbiased measurement of the acoustic scale.
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