A. Smith
A lightcone catalogue from the Millennium-XXL simulation
Smith, A.; Cole, S.; Baugh, C.; Zheng, Z.; Angulo, R.; Norberg, P.; Zehavi, I.
Authors
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
Professor Carlton Baugh c.m.baugh@durham.ac.uk
Professor
Z. Zheng
R. Angulo
Professor Peder Norberg peder.norberg@durham.ac.uk
Professor
I. Zehavi
Abstract
Future galaxy surveys require realistic mock catalogues to understand and quantify systematics in order to make precise cosmological measurements. We present a halo lightcone catalogue and halo occupation distribution (HOD) galaxy catalogue built using the Millennium-XXL simulation. The halo catalogue covers the full sky, extending to z = 2.2 with a mass resolution of ∼1011 h−1 M⊙. We use this to build a galaxy catalogue, which has an r-band magnitude limit of r < 20.0, with a median redshift of z ∼ 0.2. A Monte Carlo HOD method is used to assign galaxies to the halo lightcone catalogue, and we evolve the HODs to reproduce a target luminosity function; by construction, the luminosity function of galaxies in the mock is in agreement with the Sloan Digital Sky Survey (SDSS) at low redshifts and the Galaxy and Mass Assembly (GAMA) survey at high redshifts. A Monte Carlo method is used to assign a 0.1(g − r) colour to each galaxy, and the colour distribution of galaxies at different redshifts agrees with measurements from GAMA. The clustering of galaxies in the mock for galaxies in different magnitude and redshift bins is in good agreement with measurements from SDSS and GAMA, and the colour-dependent clustering is in reasonable agreement. We show that the baryon acoustic oscillation can be measured in the mock catalogue, and the redshift-space distortions are in agreement with measurements from SDSS illustrating that this catalogue will be useful for upcoming surveys.
Citation
Smith, A., Cole, S., Baugh, C., Zheng, Z., Angulo, R., Norberg, P., & Zehavi, I. (2017). A lightcone catalogue from the Millennium-XXL simulation. Monthly Notices of the Royal Astronomical Society, 470(4), 4646-4661. https://doi.org/10.1093/mnras/stx1432
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 7, 2017 |
Online Publication Date | Jun 12, 2017 |
Publication Date | Oct 1, 2017 |
Deposit Date | Aug 29, 2017 |
Publicly Available Date | Aug 31, 2017 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 470 |
Issue | 4 |
Pages | 4646-4661 |
DOI | https://doi.org/10.1093/mnras/stx1432 |
Public URL | https://durham-repository.worktribe.com/output/1346509 |
Files
Published Journal Article
(2.6 Mb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2017. The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
You might also like
The two-point correlation function covariance with fewer mocks
(2023)
Journal Article
The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation
(2023)
Journal Article
A sparse regression approach for populating dark matter haloes and subhaloes with galaxies
(2022)
Journal Article
Solving small-scale clustering problems in approximate light-cone mocks
(2022)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search