Dark Energy Spectroscopic Instrument (DESI)

There is a newer version of the record available.

Published 2024 | Version v1
Output management plan Open

Suppressing the sample variance of DESI-like galaxy clustering with fast simulations

Creators

  • 1. Shanghai Jiao Tong University
  • 2. ROR icon École Polytechnique Fédérale de Lausanne
  • 3. ROR icon Tata Institute of Fundamental Research

Description

Supplementary data and jupyter notebooks for the figures of the paper "Suppressing the sample variance of DESI-like galaxy clustering with fast simulations".

The file clustering_analysis.gzip contains the data for the two-point correlation function and power spectra from the AbacusSummit and FastPM galaxy catalogs. 

The file bao_fit.gzip contains the data and code fitting the BAO signal from the AbacusSummit two-point correlation function (or power spectrum) with and without the CARPool application, respectively.

 

Files

Files (66.3 MB)

Name Size Download all
md5:0ca91631b76c841078f02a0e4457c8d7
50.7 MB Download
md5:39184d513bbb26f558b7772df257d261
15.6 MB Download