Synthetic spectra for Lyman-$α$ forest analysis in the Dark Energy Spectroscopic Instrument

Hiram K. Herrera-Alcantar, Andrea Muñoz-Gutiérrez, Ting Tan, Alma X. González-Morales, Andreu Font-Ribera, Julien Guy, John Moustakas, David Kirkby, E. Armengaud, A. Bault, L. Cabayol-Garcia, J. Chaves-Montero, A. Cuceu, R. de la Cruz, L. Á. García, C. Gordon, V. Iršič, N. G. Karaçaylı, P. Montero-Camacho, G. Niz, I. Pérez-Ràfols, C. Ramírez-Pérez, C. Ravoux, M. Walther, J. Aguilar, S. Ahlen, D. Brooks, T. Claybaugh, K. Dawson, A. de la Macorra, P. Doel, J. E. Forero-Romero, E. Gaztañaga, S. Gontcho A Gontcho, K. Honscheid, R. Kehoe, T. Kisner, M. Landriau, Michael E. Levi, M. Manera, P. Martini, A. Meisner, R. Miquel, J. Nie, N. Palanque-Delabrouille, C. Poppett, M. Rezaie, G. Rossi, E. Sanchez, H. Seo, G. Tarlé, B. A. Weaver, Z. Zhou

Published 2023-12-30Version 1

Synthetic data sets are used in cosmology to test analysis procedures, to verify that systematic errors are well understood and to demonstrate that measurements are unbiased. In this work we describe the methods used to generate synthetic datasets of Lyman-$\alpha$ quasar spectra aimed for studies with the Dark Energy Spectroscopic Instrument (DESI). In particular, we focus on demonstrating that our simulations reproduces important features of real samples, making them suitable to test the analysis methods to be used in DESI and to place limits on systematic effects on measurements of Baryon Acoustic Oscillations (BAO). We present a set of mocks that reproduce the statistical properties of the DESI early data set with good agreement. Additionally, we use full survey synthetic data to forecast the BAO scale constraining power with DESI.