TY - JOUR
T1 - 3D correlations in the Lyman-α forest from early DESI data
AU - DESI Collaboration
AU - Gordon, C.
AU - Cuceu, A.
AU - Chaves-Montero, J.
AU - Font-Ribera, A.
AU - González-Morales, A. X.
AU - Aguilar, J.
AU - Ahlen, S.
AU - Armengaud, E.
AU - Bailey, S.
AU - Bault, A.
AU - Brodzeller, A.
AU - Brooks, D.
AU - Claybaugh, T.
AU - de la Cruz, R.
AU - Dawson, K.
AU - Doel, P.
AU - Forero-Romero, J. E.
AU - Gontcho, S. Gontcho A.
AU - Guy, J.
AU - Herrera-Alcantar, H. K.
AU - Iršič, V.
AU - Karaçaylı, N. G.
AU - Kirkby, D.
AU - Landriau, M.
AU - Le Guillou, L.
AU - Levi, M. E.
AU - de la Macorra, A.
AU - Manera, M.
AU - Martini, P.
AU - Meisner, A.
AU - Miquel, R.
AU - Montero-Camacho, P.
AU - Muñoz-Gutiérrez, A.
AU - Napolitano, L.
AU - Nie, J.
AU - Niz, G.
AU - Palanque-Delabrouille, N.
AU - Percival, W. J.
AU - Pieri, M.
AU - Poppett, C.
AU - Prada, F.
AU - Pérez-Ràfols, I.
AU - Ramírez-Pérez, C.
AU - Ravoux, C.
AU - Rezaie, M.
AU - Ross, A. J.
AU - Rossi, G.
AU - Sanchez, E.
AU - Schlegel, D.
AU - Zhou, Z.
N1 - Publisher Copyright:
© 2023 IOP Publishing Ltd and Sissa Medialab.
PY - 2023/11/1
Y1 - 2023/11/1
N2 - We present the first measurements of Lyman-α (Lyα) forest correlations using early data from the Dark Energy Spectroscopic Instrument (DESI). We measure the auto-correlation of Lyα absorption using 88 509 quasars at z > 2, and its cross-correlation with quasars using a further 147 899 tracer quasars at z ≳ 1.77. Then, we fit these correlations using a 13-parameter model based on linear perturbation theory and find that it provides a good description of the data across a broad range of scales. We detect the BAO peak with a signal-to-noise ratio of 3.8σ, and show that our measurements of the auto- and cross-correlations are fully-consistent with previous measurements by the Extended Baryon Oscillation Spectroscopic Survey (eBOSS). Even though we only use here a small fraction of the final DESI dataset, our uncertainties are only a factor of 1.7 larger than those from the final eBOSS measurement. We validate the existing analysis methods of Lyα correlations in preparation for making a robust measurement of the BAO scale with the first year of DESI data.
AB - We present the first measurements of Lyman-α (Lyα) forest correlations using early data from the Dark Energy Spectroscopic Instrument (DESI). We measure the auto-correlation of Lyα absorption using 88 509 quasars at z > 2, and its cross-correlation with quasars using a further 147 899 tracer quasars at z ≳ 1.77. Then, we fit these correlations using a 13-parameter model based on linear perturbation theory and find that it provides a good description of the data across a broad range of scales. We detect the BAO peak with a signal-to-noise ratio of 3.8σ, and show that our measurements of the auto- and cross-correlations are fully-consistent with previous measurements by the Extended Baryon Oscillation Spectroscopic Survey (eBOSS). Even though we only use here a small fraction of the final DESI dataset, our uncertainties are only a factor of 1.7 larger than those from the final eBOSS measurement. We validate the existing analysis methods of Lyα correlations in preparation for making a robust measurement of the BAO scale with the first year of DESI data.
KW - baryon acoustic oscillations
KW - dark energy experiments
KW - Lyman alpha forest
UR - http://www.scopus.com/inward/record.url?scp=85177486227&partnerID=8YFLogxK
U2 - 10.1088/1475-7516/2023/11/045
DO - 10.1088/1475-7516/2023/11/045
M3 - Article
AN - SCOPUS:85177486227
SN - 1475-7516
VL - 2023
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
IS - 11
M1 - 045
ER -