Alexander Smith alexander.p.smith@durham.ac.uk
PGR Student Master of Science
Solving small-scale clustering problems in approximate light-cone mocks
Smith, Alex; Cole, Shaun; Grove, Cameron; Norberg, Peder; Zarrouk, Pauline
Authors
Professor Shaun Cole shaun.cole@durham.ac.uk
Director of the Institute for Computational Cosmology
Cameron Grove cameron.grove@durham.ac.uk
PGR Student Doctor of Philosophy
Professor Peder Norberg peder.norberg@durham.ac.uk
Professor
Pauline Zarrouk
Abstract
Realistic light-cone mocks are important in the clustering analyses of large galaxy surveys. For simulations where only the snapshots are available, it is common to create approximate light-cones by joining together the snapshots in spherical shells. We assess the two-point clustering measurements of central galaxies in approximate light-cones built from the Millennium-XXL simulation, which are constructed using different numbers of snapshots. The monopole and quadrupole of the real-space correlation function is strongly boosted on small scales below 1 h−1 Mpc, due to some galaxies being duplicated at the boundaries between snapshots in the light-cone. When more snapshots are used, the total number of duplicated galaxies is approximately constant, but they are pushed to smaller separations. The effect of this in redshift space is small, as long as the snapshots are cut into shells in real space. Randomly removing duplicated galaxies is able to reduce the excess clustering signal. Including satellite galaxies will reduce the impact of the duplicates, since many small-scale pairs come from satellites in the same halo. Galaxies that are missing from the light-cone at the boundaries can be added to the light-cone by having a small overlap between each shell. This effect will impact analyses that use very small-scale clustering measurements, and when using mocks to test the impact of fibre collisions.
Citation
Smith, A., Cole, S., Grove, C., Norberg, P., & Zarrouk, P. (2022). Solving small-scale clustering problems in approximate light-cone mocks. Monthly Notices of the Royal Astronomical Society, 516(1), 1062 - 1071. https://doi.org/10.1093/mnras/stac2219
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 2, 2022 |
Online Publication Date | Aug 6, 2022 |
Publication Date | 2022 |
Deposit Date | Nov 17, 2022 |
Publicly Available Date | Nov 18, 2022 |
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 | 516 |
Issue | 1 |
Pages | 1062 - 1071 |
DOI | https://doi.org/10.1093/mnras/stac2219 |
Public URL | https://durham-repository.worktribe.com/output/1185891 |
Files
Published Journal Article (Advance online version)
(981 Kb)
PDF
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
Copyright Statement
Advance online version This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
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
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