Discovery of Strongly Lensed Quasars in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)

TL;DR

This paper reports the discovery of five new doubly-imaged lensed quasars using the CFIS survey data, demonstrating an effective method for identifying small-separation lensed quasars with high recovery rate.

Contribution

The study introduces a novel approach combining deep imaging and color selection to efficiently discover small-separation lensed quasars in the CFIS survey.

Findings

Discovered five new doubly lensed quasars with redshifts 1.21 to 3.36.

Achieved an 83% recovery rate of known bright lenses in the CFIS footprint.

Method predicts a complete discovery of small-separation lenses below z=2.7 within CFIS data.

Abstract

We report the discovery of five new doubly-imaged lensed quasars from the first 2500 square degrees of the ongoing Canada-France Imaging Survey (CFIS), which is a component of the Ultraviolet Near Infrared Optical Northern Survey (UNIONS), selected from initial catalogues of either Gaia pairs or MILLIQUAS quasars. We take advantage of the deep, 0.6'' median-seeing $r$-band imaging of CFIS to confirm the presence of multiple point sources with similar colour of $u-r$, via convolution of the Laplacian of the point spread function. Requiring similar-colour point sources with flux ratios less than 2.5 mag in $r$-band, reduces the number of candidates from 256314 to 7815. After visual inspection we obtain 30 high-grade candidates, and prioritise spectroscopic follow-up for those showing signs of a lensing galaxy upon subtraction of the point sources. We obtain long-slit spectra for 18 candidates with ALFOSC on the 2.56-m Nordic Optical Telescope (NOT), confirming five new doubly lensed quasars with $1.21<z<3.36$ and angular separations from 0.8'' to 2.5''. One additional system is a probable lensed quasar based on the CFIS imaging and existing SDSS spectrum. We further classify six objects as nearly identical quasars -- still possible lenses but without the detection of a lensing galaxy. Given our recovery rate ($83\%$) of existing optically bright lenses within the CFIS footprint, we expect that a similar strategy, coupled with $u-r$ colour-selection from CFIS alone, will provide an efficient and complete discovery of small-separation lensed quasars of source redshifts below $z=2.7$ within the CFIS $r$-band magnitude limit of 24.1 mag.