3D correlations in the Lyman-α forest from early DESI data
/ Authors
Calum K. Gordon, A. Cuceu, J. Chaves-Montero, A. Font-Ribera, A. X. Gonz'alez-Morales, J. Aguilar, S. Ahlen, E. Armengaud, S. Bailey, A. Bault
and 49 more authors
A. Brodzeller, D. Brooks, T. Claybaugh, R. D. L. Cruz, K. Dawson, P. Doel, J. Forero-Romero, S. Gontcho, J. Guy, H. Herrera-Alcantar, V. Irvsivc, N. G. Karaccayli, D. Kirkby, M. Landriau, L. Guillou, M. Levi, A. Macorra, M. Manera, P. Martini, A. Meisner, R. Miquel, P. Montero-Camacho, A. Munoz-Guti'errez, L. Napolitano, J. Nie, G. Niz, N. Palanque-Delabrouille, W. Percival, M. Pieri, C. Poppett, F. Prada, I. P'erez-Rafols, C. Ram'irez-P'erez, C. Ravoux, M. Rezaie, A. Ross, G. Rossi, E. Sanchez, D. Schlegel, M. Schubnell, H. Seo, F. Sinigaglia, T. Tan, G. Tarl'e, M. Walther, B. Weaver, C. Yéche, Z. Zhou, H. Zou
/ Abstract
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.
Journal: Journal of Cosmology and Astroparticle Physics