Optimal strategies for identifying quasars in DESI
James Farr, Andreu Font-Ribera, Andrew Pontzen

TL;DR
This paper evaluates machine learning classifiers for quasar identification in DESI, demonstrating that combining QuasarNET with existing methods significantly improves high-redshift quasar detection accuracy and reduces contamination.
Contribution
It introduces the use of QuasarNET for DESI quasar classification and shows how combining it with redrock enhances performance over current methods.
Findings
QuasarNET identifies ~99% of high-z QSOs from single exposures.
Combined classifiers achieve >99.5% high-z QSO detection.
Contamination in QSO catalogues is reduced below 0.5%.
Abstract
As spectroscopic surveys continue to grow in size, the problem of classifying spectra targeted as quasars (QSOs) will need to move beyond its historical reliance on human experts. Instead, automatic classifiers will increasingly become the dominant classification method, leaving only small fractions of spectra to be visually inspected in ambiguous cases. In order to maximise classification accuracy, making best use of available classifiers will be of great importance, particularly when looking to identify and eliminate distinctive failure modes. In this work, we demonstrate that the machine learning-based classifier QuasarNET will be of use for future surveys such as the Dark Energy Spectroscopic Instrument (DESI), comparing its performance to the DESI pipeline classifier redrock. During the first of four passes across its footprint DESI will need to select high- () QSOs…
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