Discovery of Strongly Lensed Quasars in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS)
arXiv:2110.09535 · doi:10.1051/0004-6361/202142389
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 -band imaging of CFIS to confirm the presence of multiple point sources with similar colour of , via convolution of the Laplacian of the point spread function. Requiring similar-colour point sources with flux ratios less than 2.5 mag in -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 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 () of existing optically bright lenses within the CFIS footprint, we expect that a similar strategy, coupled with colour-selection from CFIS alone, will provide an efficient and complete discovery of small-separation lensed quasars of source redshifts below within the CFIS -band magnitude limit of 24.1 mag.
15 pages, 8 figures
References in corpus (20)
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- MegaPipe: the MegaCam image stacking pipeline at the Canadian Astronomical Data Centre
- The Sloan Digital Sky Survey Quasar Lens Search. I. Candidate Selection Algorithm
- The Million Quasars (Milliquas) Catalogue, v8
- The Canada-France Imaging Survey: First results from the u-band component
- The Sloan Digital Sky Survey Quasar Lens Search. II. Statistical Lens Sample from the Third Data Release
- The Sloan Digital Sky Survey Quasar Lens Search. III. Constraints on Dark Energy from the Third Data Release Quasar Lens Catalog
- The Canada-France Imaging Survey: Reconstructing the Milky Way Star Formation History from its White Dwarf Population
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). VI. Crowdsourced lens finding with Space Warps
- Discovery of a close-separation binary quasar at the heart of a z~0.2 merging galaxy and its implications for low-frequency gravitational waves
- A hidden population of high-redshift double quasars unveiled by astrometry
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). V. Group-to-cluster scale lens search from the HSC-SSP Survey
- The Sloan Digital Sky Survey Quasar Lens Search. IV. Statistical Lens Sample from the Fifth Data Release
- Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). IV. Lensed quasar search in the HSC survey
- CHITAH: Strong-gravitational-lens hunter in imaging surveys
- A quasar-based supermassive black hole binary population model: implications for the gravitational-wave background
- Survey of Gravitationally lensed Objects in HSC Imaging (SuGOHI) -- VII. Discovery and Confirmation of Three Strongly Lensed Quasars
- J17218842: a gravitationally lensed binary quasar with a proximate damped Lyman- absorber
- Exploiting flux ratio anomalies to probe warm dark matter in future large scale surveys
- A Redshift for the First Einstein Ring, MG 1131+0456
Cited by in corpus (4)
- Gravitationally lensed quasars in Gaia -- IV. 150 new lenses, quasar pairs, and projected quasars
- Streamlined Lensed Quasar Identification in Multiband Images via Ensemble Networks
- Accelerating lensed quasar discovery and modeling with physics-informed variational autoencoders
- Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey