Atacama Cosmology Telescope DR6 and DESI: Structure growth measurements from the cross-correlation of DESI legacy imaging galaxies and CMB lensing from ACT DR6 and Planck PR4

Qu, Frank J., Hang, Qianjun, Farren, Gerrit, Bolliet, Boris, Aguilar, Jessica Nicole, Ahlen, Steven, Alam, Shadab, Brooks, David, Cai, Yan-Chuan, Calabrese, Erminia ORCID: https://orcid.org/0000-0003-0837-0068, Claybaugh, Todd, de la Macorra, Axel, Devlin, Mark J., Doel, Peter, Embil-Villagra, Carmen, Ferraro, Simone, Font-Ribera, Andreu, Forero-Romero, Jaime E., Gaztañaga, Enrique, Gluscevic, Vera, Gontcho, Satya Gontcho A., Gutierrez, Gaston, Howlett, Cullan, Kehoe, Robert, Kim, Joshua, Kremin, Anthony, Lambert, Andrew, Landriau, Martin, Le Guillou, Laurent, Levi, Michael, Louis, Thibaut, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Newman, Jeffrey A., Niz, Gustavo, Peacock, John A., Percival, Will, Poppett, Claire, Prada, Francisco, Pérez-Ràfols, Ignasi, Rossi, Graziano, Sanchez, Eusebio, Schlegel, David, Sehgal, Neelima, Shaikh, Shabbir, Sherwin, Blake, Sifón, Cristóbal, Schubnell, Michael, Sprayberry, David, Tarlé, Gregory, Weaver, Benjamin Alan, Wollack, Edward J. and Zou, Hu 2025. Atacama Cosmology Telescope DR6 and DESI: Structure growth measurements from the cross-correlation of DESI legacy imaging galaxies and CMB lensing from ACT DR6 and Planck PR4. Physical Review D (particles, fields, gravitation, and cosmology) 111 (10) , 103503. 10.1103/physrevd.111.103503

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Abstract

We measure the growth of cosmic density fluctuations on large scales and across the redshift range 0.3<0.8 through galaxy clustering and the cross-correlation of the ACT data release 6 cosmic microwave background (CMB) lensing map and galaxies from the Dark Energy Spectroscopic Instrument Legacy Survey, using three galaxy samples spanning the redshifts of 0.3≲z≲0.45, 0.45≲z≲0.6, 0.6≲z≲0.8. We adopt a scale cut where nonlinear effects are negligible, so that the cosmological constraints are derived from the linear regime. We determine the amplitude of matter fluctuations over all three redshift bins using Atacama Cosmology Telescope (ACT) data alone to be S8≡σ8(Ωm/0.3)0.5=0.772±0.040 in a joint analysis combining the three redshift bins and ACT lensing alone. Using a combination of ACT and data we obtain S8=0.765±0.032. The lowest redshift bin used is the least constraining and exhibits a ∼2σ tension with the other redshift bins; thus we also report constraints excluding the first redshift bin, giving S8=0.785±0.033 for the combination of ACT and . This result is in excellent agreement at the 0.3σ level with measurements from galaxy lensing, but is 1.8σ lower than predictions based on primary CMB data. Understanding whether this hint of discrepancy in the growth of structure at low redshifts arises from a fluctuation, from systematics in data, or from new physics is a high priority for forthcoming CMB lensing and galaxy cross-correlation analyses. Published by the American Physical Society 2025

Item Type:	Article
Date Type:	Published Online
Status:	Published
Schools:	Schools > Physics and Astronomy
Additional Information:	License information from Publisher: LICENSE 1: URL: https://creativecommons.org/licenses/by/4.0/, Start Date: 2025-05-02
Publisher:	American Physical Society
ISSN:	2470-0010
Date of First Compliant Deposit:	2 June 2025
Date of Acceptance:	10 April 2025
Last Modified:	02 Jun 2025 11:15
URI:	https://orca.cardiff.ac.uk/id/eprint/178645

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