UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space

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Main Authors: Goh, L. W. K., Guerrini, S., Daley, C., Hervas-Peters, F., Kilbinger, M., Wittje, A., Murray, C., Fabbro, S., Hildebrandt, H., Hudson, M. J., van Waerbeke, L., Wright, A. H., de Boer, T., Cuillandre, J. -C., Magnier, E., McConnachie, A. W.
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Published: 2026
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author Goh, L. W. K.
Guerrini, S.
Daley, C.
Hervas-Peters, F.
Kilbinger, M.
Wittje, A.
Murray, C.
Fabbro, S.
Hildebrandt, H.
Hudson, M. J.
van Waerbeke, L.
Wright, A. H.
de Boer, T.
Cuillandre, J. -C.
Magnier, E.
McConnachie, A. W.
author_facet Goh, L. W. K.
Guerrini, S.
Daley, C.
Hervas-Peters, F.
Kilbinger, M.
Wittje, A.
Murray, C.
Fabbro, S.
Hildebrandt, H.
Hudson, M. J.
van Waerbeke, L.
Wright, A. H.
de Boer, T.
Cuillandre, J. -C.
Magnier, E.
McConnachie, A. W.
contents We present the first cosmological constraints from the cosmic shear analysis of the UNIONS-3500 weak lensing galaxy catalogue in configuration space. The Ultraviolet Near Infrared Optical Northern Survey (UNIONS) is the largest and deepest photometric survey of the northern hemisphere to date, with the UNIONS-3500 catalogue using high-quality $r$-band imaging across 3500 deg2 of the sky. We perform a 2D cosmic shear analysis with a single tomographic bin, using the two-point correlation function (2PCF) statistic. Assuming a flat LCDM model, we obtain constraints on the clustering amplitude of S_8 = 0.831^{+0.067}_{-0.078}, which is consistent with constraints from Planck CMB measurements and precedent cosmic shear results within 1sigma. We outline the construction of our cosmological inference pipeline, including the estimation of the source redshift distribution, shear calibration, and covariance matrix, and describe methodologies for the mitigation of systematic effects arising from PSF systematics and B-modes. We demonstrate that our results are robust to variations in analysis choices, including scale cuts, prior ranges, and nonlinear modelling. This paper is part of a coordinated release which collectively demonstrates the maturity and readiness of UNIONS to deliver competitive cosmological results, positioning it as a key stepping stone towards the forthcoming era of Stage IV weak lensing experiments.
format Preprint
id arxiv_https___arxiv_org_abs_2605_13547
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space
Goh, L. W. K.
Guerrini, S.
Daley, C.
Hervas-Peters, F.
Kilbinger, M.
Wittje, A.
Murray, C.
Fabbro, S.
Hildebrandt, H.
Hudson, M. J.
van Waerbeke, L.
Wright, A. H.
de Boer, T.
Cuillandre, J. -C.
Magnier, E.
McConnachie, A. W.
Cosmology and Nongalactic Astrophysics
We present the first cosmological constraints from the cosmic shear analysis of the UNIONS-3500 weak lensing galaxy catalogue in configuration space. The Ultraviolet Near Infrared Optical Northern Survey (UNIONS) is the largest and deepest photometric survey of the northern hemisphere to date, with the UNIONS-3500 catalogue using high-quality $r$-band imaging across 3500 deg2 of the sky. We perform a 2D cosmic shear analysis with a single tomographic bin, using the two-point correlation function (2PCF) statistic. Assuming a flat LCDM model, we obtain constraints on the clustering amplitude of S_8 = 0.831^{+0.067}_{-0.078}, which is consistent with constraints from Planck CMB measurements and precedent cosmic shear results within 1sigma. We outline the construction of our cosmological inference pipeline, including the estimation of the source redshift distribution, shear calibration, and covariance matrix, and describe methodologies for the mitigation of systematic effects arising from PSF systematics and B-modes. We demonstrate that our results are robust to variations in analysis choices, including scale cuts, prior ranges, and nonlinear modelling. This paper is part of a coordinated release which collectively demonstrates the maturity and readiness of UNIONS to deliver competitive cosmological results, positioning it as a key stepping stone towards the forthcoming era of Stage IV weak lensing experiments.
title UNIONS-3500 Weak Lensing: III. 2D Cosmological Constraints in Configuration Space
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2605.13547