Searching for strong lensing by late-type galaxies in UNIONS

dc.contributor.authorBarroso, Javier A. Acevedo
dc.contributor.authorClément, Benjamin
dc.contributor.authorCourbin, Frederic
dc.contributor.authorGavazzi, Raphael
dc.contributor.authorLemon, Cameron
dc.contributor.authorRojas, Karina
dc.contributor.authorScott, Douglas
dc.contributor.authorGwyn, Stephen
dc.contributor.authorHammer, Francois
dc.contributor.authorHudson, Michael J.
dc.contributor.authorMagnier, Eugene A.
dc.date.accessioned2026-06-03T06:45:03Z
dc.date.issued2026
dc.description.abstractRecent wide-field galaxy surveys have led to an explosion in the number of galaxy-scale strong gravitational lens candidates. However, the vast majority of them feature massive luminous red galaxies as the main deflectors, with late-type galaxies being vastly under-represented. This work presents a dedicated search for lensing by edge-on late-type galaxies in the Ultraviolet Near Infrared Optical Northern Survey (UNIONS). The search covers 3600 deg 2 of r -band observations taken from the Canada-France-Hawaii Telescope. We considered all sources with magnitudes in the range 17 < r < 20.5, without any colour pre-selection, yielding a parent sample of seven million sources. We characterised our parent sample via the visual inspection of 120 000 sources selected at random. From it, we estimate, with a 68% confidence interval, that 1 in every 30 000 sources is an edge-on lens candidate, with at least eight high-quality candidates in the parent sample. This corresponds to one candidate per 17 000 edge-on late-type galaxies. Our search relied on a convolutional neural network (CNN) to select a reduced sample of candidates, which we followed with a visual inspection to curate the final sample. The CNN was trained from scratch using simulated r -band observations of edge-on lenses, and real observations of non-lenses. We found 61 good edge-on lens candidates using the CNN. Moreover, combining the CNN candidates with those found serendipitously and those identified while characterising the parent sample, we discovered 4 grade A, 20 grade B, and 58 grade C edge-on lens candidates, effectively doubling the known sample of these systems. We also discovered 16 grade A, 16 grade B, and 18 grade C lens candidates of other types. Finally, based on the characterisation of the parent sample, we estimate that our search found around 60% of the bright grade A and B edge-on lens candidates within the parent sample.
dc.identifier.doi10.1051/0004-6361/202554555
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.urihttps://irf.fhnw.ch/handle/11645/56954
dc.issueA146
dc.language.isoen
dc.publisherEDP Sciences
dc.relation.ispartofAstronomy & Astrophysics
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subject.ddc520 - Astronomie, Kartografie
dc.titleSearching for strong lensing by late-type galaxies in UNIONS
dc.type01A - Beitrag in wissenschaftlicher Zeitschrift
dc.volume706
dspace.entity.typePublication
fhnw.InventedHereYes
fhnw.ReviewTypepeer-reviewed
fhnw.oastatus.auroraVersion: Published *** Embargo: None *** Licence: CC BY *** URL: https://v2.sherpa.ac.uk/id/publication/11142
fhnw.openAccessCategoryGold
fhnw.publicationStatePublished
fhnw.targetcollectionb508cce9-5084-49ae-a565-d8e5c348c3ab
relation.isAuthorOfPublicationb958796a-5dea-4ee5-b8cd-8f186e7ef908
relation.isAuthorOfPublication.latestForDiscoveryb958796a-5dea-4ee5-b8cd-8f186e7ef908
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