Skip to main navigation Skip to search Skip to main content

Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS

Benjamin R. Granett, Ginevra Favole, Antonio D. Montero-Dorta, Enzo Branchini, Luigi Guzzo, Sylvain de la Torre

Research output: Contribution to journalArticlepeer-review

108 Downloads (Pure)

Abstract

We test the history of structure formation from redshift 1 to today by matching galaxies from VIPERS and SDSS with dark matter haloes in the MultiDark SMDPL N-body simulation. We first show that the standard subhalo abundance matching (SHAM) recipe implemented with MultiDark characterizes the clustering of galaxies well both at redshift 0 for SDSS and at redshift 1 for VIPERS. This is an important validation of the SHAM model at high redshift. We then remap the simulation timesteps to test alternative growth histories and infer the growth index $\gamma=0.6\pm0.3$. This analysis demonstrates the power of using N-body simulations to forward model galaxy surveys for cosmological inference.
Original languageEnglish
Pages (from-to)653-662
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume489
Issue number1
Early online date20 Aug 2019
DOIs
Publication statusPublished - 1 Oct 2019

Keywords

  • astro-ph.CO
  • galaxies: statistics
  • cosmology: observations
  • large-scale structure of Universe

Fingerprint

Dive into the research topics of 'Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS'. Together they form a unique fingerprint.

Cite this