We present an alternative measurement of the Baryon Acoustic Oscillation (BAO) using the Legendre multipole representation of the Lyman-𝛼 forest correlation functions from the second data release (DR2) of the Dark Energy Spectroscopic Instrument survey. Compressing the autocorrelation and cross-correlation functions into Legendre multipoles yields a positive-definite covariance matrix without any smoothing—unlike the baseline DR2 analysis—thanks to a significantly reduced data vector size. We introduce the statistical corrections required to debias the finite-sample covariance matrix estimate and demonstrate that monopole and quadrupole terms for both autocorrelations and cross-correlations can be used even when the correlation functions are distorted by continuum errors and contaminated by metals. This formalism has slightly diminished the constraining power of the BAO scale, while considerably weakening constraints on nuisance parameters. We measure the isotropic BAO scale with 0.93% precision at 𝑧eff =2.35 , the Hubble parameter 𝐻⁡(𝑧eff)=(239.5±3.4)⁢(147.09  Mpc/𝑟𝑑) km s−1 Mpc−1 , and the transverse comoving distance 𝐷𝑀⁡(𝑧eff)=(5.80±0.10)⁢(𝑟𝑑/147.09  Mpc) Gpc for a given value of the sound horizon (𝑟𝑑 ). Our BAO results are entirely consistent with the baseline DR2 analysis.

DESI DR2 baryon acoustic oscillations from the Lyman alpha forest multipoles / N.G. Karaçayl��, A.C.. - In: PHYSICAL REVIEW D. - ISSN 2470-0010. - 114:4(2026 Aug 11), pp. 043518.1-043518.15. [10.1103/yl3v-cyck]

DESI DR2 baryon acoustic oscillations from the Lyman alpha forest multipoles

D. Bianchi;G. Rossi
Membro del Collaboration Group
;
2026

Abstract

We present an alternative measurement of the Baryon Acoustic Oscillation (BAO) using the Legendre multipole representation of the Lyman-𝛼 forest correlation functions from the second data release (DR2) of the Dark Energy Spectroscopic Instrument survey. Compressing the autocorrelation and cross-correlation functions into Legendre multipoles yields a positive-definite covariance matrix without any smoothing—unlike the baseline DR2 analysis—thanks to a significantly reduced data vector size. We introduce the statistical corrections required to debias the finite-sample covariance matrix estimate and demonstrate that monopole and quadrupole terms for both autocorrelations and cross-correlations can be used even when the correlation functions are distorted by continuum errors and contaminated by metals. This formalism has slightly diminished the constraining power of the BAO scale, while considerably weakening constraints on nuisance parameters. We measure the isotropic BAO scale with 0.93% precision at 𝑧eff =2.35 , the Hubble parameter 𝐻⁡(𝑧eff)=(239.5±3.4)⁢(147.09  Mpc/𝑟𝑑) km s−1 Mpc−1 , and the transverse comoving distance 𝐷𝑀⁡(𝑧eff)=(5.80±0.10)⁢(𝑟𝑑/147.09  Mpc) Gpc for a given value of the sound horizon (𝑟𝑑 ). Our BAO results are entirely consistent with the baseline DR2 analysis.
Settore PHYS-05/A - Astrofisica, cosmologia e scienza dello spazio
11-ago-2026
Article (author)
File in questo prodotto:
File Dimensione Formato  
2603.04281v2.pdf

accesso aperto

Tipologia: Pre-print (manoscritto inviato all'editore)
Licenza: Altro
Dimensione 1.46 MB
Formato Adobe PDF
1.46 MB Adobe PDF Visualizza/Apri
Pubblicazioni consigliate

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/1272843
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? ND
  • OpenAlex ND
social impact