Discovering strongly lensed quasar candidates with catalogue-based methods from DESI Legacy Surveys
Zizhao He, Nan Li, Xiaoyue Cao, Rui Li, Hu Zou, Simon Dye

TL;DR
This paper presents a catalogue-based method to identify candidate strongly lensed quasars in DESI Legacy Surveys, significantly expanding the sample for cosmological measurements like the Hubble constant.
Contribution
The authors develop a novel catalogue-based approach using spatial and color similarity to discover 620 new candidate lensed quasars in DESI data.
Findings
Identified 620 new candidate lensed quasars.
Method combines spatial clustering and color similarity filtering.
Candidates will be validated with spectroscopic and photometric data.
Abstract
The Hubble tension, revealed by a discrepancy between measurements of the Hubble-Lemaitre constant from early- and local-Universe observations, is one of the most significant problems in modern cosmology. In order to better understand the origin of this mismatch, independent techniques to measure , such as strong lensing time delays, are required. Notably, the sample size of such systems is key to minimising statistical uncertainties and cosmic variance, which can be improved by exploring the datasets of large-scale sky surveys like DESI (Dark Energy Spectroscopic Instrument). We identify possible strong lensing time-delay systems within DESI by selecting candidate multiply imaged lensed quasars from a catalogue of 24,440,816 candidate QSOs contained in the 9th data release of the DESI Legacy Imaging Surveys (DESI-LS). Using a friend-of-friends-like algorithm on…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Astronomical Observations and Instrumentation
