Detailed Record



Target Selection and Validation of DESI Quasars


Abstract The Dark Energy Spectroscopic Instrument (DESI) survey will measure large-scale structures using quasars as direct tracers of dark matter in the redshift range 0.9 < z < 2.1 and using Ly α forests in quasar spectra at z > 2.1. We present several methods to select candidate quasars for DESI, using input photometric imaging in three optical bands ( g , r , z ) from the DESI Legacy Imaging Surveys and two infrared bands (W1, W2) from the Wide-field Infrared Survey Explorer. These methods were extensively tested during the Survey Validation of DESI. In this paper, we report on the results obtained with the different methods and present the selection we optimized for the DESI main survey. The final quasar target selection is based on a random forest algorithm and selects quasars in the magnitude range of 16.5 < r < 23. Visual selection of ultra-deep observations indicates that the main selection consists of 71% quasars, 16% galaxies, 6% stars, and 7% inconclusive spectra. Using the spectra based on this selection, we build an automated quasar catalog that achieves a fraction of true QSOs higher than 99% for a nominal effective exposure time of ∼1000 s. With a 310 deg −2 target density, the main selection allows DESI to select more than 200 deg −2 quasars (including 60 deg −2 quasars with z > 2.1), exceeding the project requirements by 20%. The redshift distribution of the selected quasars is in excellent agreement with quasar luminosity function predictions.
Authors Edmond Chaussidon ORCID , Ch Yèche ORCID , N. Palanque‐Delabrouille ORCID , David Alexander ORCID , Jinyi Yang ORCID , S. P. Ahlen ORCID , S. Bailey ORCID , D. Brooks ORCID , Zheng Cai ORCID , Solène Chabanier ORCID , Tamara M. Davis ORCID , Kyle Dawson ORCID , Axel de la Macorra ORCID , Arjun Dey ORCID , Biprateep Dey ORCID , Sarah Eftekharzadeh ORCID , Daniel J. Eisenstein ORCID , Kevin Fanning ORCID , Andreu Font-Ribera ORCID , E. Gaztañaga ORCID , Satya Gontcho A Gontcho ORCID , Alma X. González‐Morales ORCID , J. Guy ORCID , H. K. Herrera-Alcantar ORCID , K. Honscheid ORCID , Mustapha Ishak , Linhua Jiang ORCID , S. Juneau ORCID , R. Kehoe ORCID , T. S. Kisner ORCID , András Kovács ORCID , Anthony Kremin ORCID , Ting-Wen Lan ORCID , Martin Landriau ORCID , L. Le Guillou ORCID , Michael Levi , C. Magneville , Paul Martini ORCID , Aaron M. Meisner ORCID , John Moustakas ORCID , A. Muñoz-Gutiérrez ORCID , Adam D. Myers University of Wyoming , Jeffrey A. Newman ORCID , Jundan Nie ORCID , Will J. Percival ORCID , Claire Poppett , Francisco Prada ORCID , Anand Raichoor ORCID , Corentin Ravoux ORCID , Ashley J. Ross ORCID , Edward F. Schlafly ORCID , David J. Schlegel ORCID , Ting Tan ORCID , G. Tarlé ORCID , Rongpu Zhou ORCID , Zhimin Zhang ORCID , Hu Zou ORCID
Journal Info IOP Publishing | The Astrophysical Journal , vol: 944 , iss: 1 , pages: 107 - 107
Publication Date 2/1/2023
ISSN 0004-637X
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/1538-4357/acb3c2
KeywordsKeyword Image Temporal Noise Analysis (Score: 0.480284)