The Dark Energy Spectroscopic Instrument: one-dimensional power spectrum from first Ly α forest samples with Fast Fourier Transform

DESI Collaboration, Corentin Ravoux, Marie Lynn Abdul Karim, Eric Armengaud, Michael Walther, Naim Göksel Karaçayll, Paul Martini, Julien Guy, Jessica Nicole Aguilar, Steven Ahlen, Stephen Bailey, Julian Bautista, Sergio Felipe Beltran, David Brooks, Laura Cabayol-Garcia, Solène Chabanier, Edmond Chaussidon, Jonás Chaves-Montero, Kyle Dawson, Rodrigo De La CruzAxel De La MacOrra, Peter Doel, Kevin Fanning, Andreu Font-Ribera, Jaime Forero-Romero, Satya Gontcho A. Gontcho, Alma X. Gonzalez-Morales, Calum Gordon, Hiram K. Herrera-Alcantar, Klaus Honscheid, Vid Iršič, Mustapha Ishak, Robert Kehoe, Theodore Kisner, Anthony Kremin, Martin Landriau, Laurent Le Guillou, Michael Levi, Zarija Lukić, Christophe Magneville, Aaron Meisner, Ramon Miquel, John Moustakas, Eva Maria Mueller, Andrea Muñoz-Gutierrez, Lucas Napolitano, Jundan Nie, Gustavo Niz, Nathalie Palanque-Delabrouille, Will Percival, Ignasi Perez-Ràfols

Research output: Contribution to journalArticlepeer-review

32 Citations (Scopus)

Abstract

We present the one-dimensional Ly α forest power spectrum measurement using the first data provided by the Dark Energy Spectroscopic Instrument (DESI). The data sample comprises 26 330 quasar spectra, at redshift z > 2.1, contained in the DESI Early Data Release and the first 2 months of the main survey. We employ a Fast Fourier Transform (FFT) estimator and compare the resulting power spectrum to an alternative likelihood-based method in a companion paper. We investigate methodological and instrumental contaminants associated with the new DESI instrument, applying techniques similar to previous Sloan Digital Sky Survey (SDSS) measurements. We use synthetic data based on lognormal approximation to validate and correct our measurement. We compare our resulting power spectrum with previous SDSS and high-resolution measurements. With relatively small number statistics, we successfully perform the FFT measurement, which is already competitive in terms of the scale range. At the end of the DESI survey, we expect a five times larger Ly α forest sample than SDSS, providing an unprecedented precise one-dimensional power spectrum measurement.
Original languageEnglish
Pages (from-to)5118-5140
Number of pages23
JournalMonthly Notices of the Royal Astronomical Society (MNRAS)
Volume526
Issue number4
Early online date5 Oct 2023
DOIs
Publication statusPublished - 31 Dec 2023

Keywords

  • cosmology: observations
  • intergalactic medium
  • large-scale structure of Universe

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