Validation of the DESI DR2 measurements of baryon acoustic oscillations from galaxies and quasars
U. Andrade, E. Paillas, J. Mena-Fernández, Qinxun Li, Ashley J. Ross, S. Nadathur, M. Rashkovetskyi, A. Pérez-Fernández, Hee‐Jong Seo, Nicole M. Sanders, O. Alves, Xinyi Chen, N. Deiosso, Arnaud de Mattia, Martin White, M. Karim, S. P. Ahlen, E. Armengaud, Alejandro Avilés, P. Bansal, Jayashree Behera, D. Bianchi, S. Brieden, A. Brodzeller, D. Brooks, E. Burtin, R. Calderón, Rebecca Canning, A. Carnero Rosell, Lidia Casas, F. J. Castander, M. Charles, E. Chaussidon, J. Chaves-Montero, T. Claybaugh, Shaun Cole, Andrew P. Cooper, Andrei Cuceu, Kyle Dawson, Axel de la Macorra, J. Della Costa, Arjun Dey, Biprateep Dey, Z. Ding, P. Doel, Daniel J. Eisenstein, Willem Elbers, E. Fernández-García, Simone Ferraro, Andreu Font-Ribera, J. E. Forero-Romero, C. García-Quintero, Lehman H. Garrison, E. Gaztañaga, Héctor Gil-Marín, Satya Gontcho A Gontcho, Alma X. González‐Morales, C. Gordon, G. Gutiérrez, J. Guy, ChangHoon Hahn, Song He, H. K. Herrera-Alcantar, K. Honscheid, Cullan Howlett, Dragan Huterer, Mustapha Ishak, S. Juneau, R. Kehoe, D. Kirkby, Theodore Kisner, Anthony Kremin, O. Lahav, C. Lamman, Martin Landriau, L. Le Guillou, Alexie Leauthaud, M. E. Levi, C. Magneville, Marc Manera, Paul Martini, William L. Matthewson, Aaron Meisner, R. Miquel, John Moustakas, A. Muñoz-Gutiérrez, D. Muñoz-Santos, Adam D. Myers, L. Napolitano, Jeffrey A. Newman, H. E. Noriega, N. Palanque‐Delabrouille, Jiaming Pan, Will J. Percival, Ignasi Pérez-Ràfols, C. Poppett, Francisco Prada, Anand Raichoor, C. Ramírez-Pérez, C. Ravoux
Abstract
The Dark Energy Spectroscopic Instrument (DESI) Data Release 2 (DR2) galaxy and quasar clustering data represents a significant expansion of data from Data Release 1 (DR1), providing improved statistical precision in baryon acoustic oscillation (BAO) constraints across multiple tracers, including bright galaxies, luminous red galaxies, emission line galaxies, and quasars. In this paper, we validate the BAO analysis of DR2. We present the results of robustness tests on the blinded DR2 data and, after unblinding, consistency checks on the unblinded DR2 data. All results are compared with those obtained from a suite of mock catalogs that replicate the selection and clustering properties of the DR2 sample. We confirm the consistency of DR2 BAO measurements with DR1 while achieving a reduction in statistical uncertainties due to the increased survey volume and completeness. The combined BAO precision, including both statistical and systematic errors, improves from <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mo>∼</a:mo> <a:mn>0.52</a:mn> <a:mo>%</a:mo> </a:math> in DR1 to 0.30% in DR2—a factor of 1.7 gain. We assess the impact of analysis choices, including different data vectors (correlation function vs power spectrum), modeling approaches and systematics treatments, and an assumption of the Gaussian likelihood, finding that our BAO constraints are stable across these variations and assumptions with a few minor refinements to the baseline setup of the DR1 BAO analysis. We summarize a series of pre-unblinding tests that confirmed the readiness of our analysis pipeline, the final systematic errors, and the DR2 BAO analysis baseline. The successful completion of these tests led to the unblinding of the DR2 BAO measurements, ultimately leading to the DESI DR2 cosmological analysis, with their implications for the expansion history of the Universe and the nature of dark energy presented in the DESI key paper (companion paper).