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Made available in DSpace on 2022-04-29T08:40:07Z (GMT). No. of bitstreams: 0 Previous issue date: 2022-04-01
We constrain the matter density ωm and the amplitude of density fluctuations σ8 within the ΛCDM cosmological model with shear peak statistics and angular convergence power spectra using mass maps constructed from the first three years of data of the Dark Energy Survey (DES Y3). We use tomographic shear peak statistics, including cross-peaks: peak counts calculated on maps created by taking a harmonic space product of the convergence of two tomographic redshift bins. Our analysis follows a forward-modelling scheme to create a likelihood of these statistics using N-body simulations, using a Gaussian process emulator. We take into account the uncertainty from the remaining, largely unconstrained ΛCDM parameters (ωb, ns, and h). We include the following lensing systematics: multiplicative shear bias, photometric redshift uncertainty, and galaxy intrinsic alignment. Stringent scale cuts are applied to avoid biases from unmodelled baryonic physics. We find that the additional non-Gaussian information leads to a tightening of the constraints on the structure growth parameter yielding S8 σ8√Ωm/0.3=0.797-0.013+0.015 (68 per cent confidence limits), with a precision of 1.8 per cent, an improvement of 38 per cent compared to the angular power spectra only case. The results obtained with the angular power spectra and peak counts are found to be in agreement with each other and no significant difference in S8 is recorded. We find a mild tension of 1.5 σ between our study and the results from Planck 2018, with our analysis yielding a lower S8. Furthermore, we observe that the combination of angular power spectra and tomographic peak counts breaks the degeneracy between galaxy intrinsic alignment AIA and S8, improving cosmological constraints. We run a suite of tests concluding that our results are robust and consistent with the results from other studies using DES Y3 data.
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Department of Physics and Astronomy University of Pennsylvania
Department of Physics and Astronomy University College London, Gower Street
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Kavli Institute for Cosmological Physics University of Chicago
Department of Physics and Astronomy Pevensey Building University of Sussex
Laboratoire de Physique de l'Ecole Normale Superieure Ens Universite Psl Cnrs Sorbonne Universite Université de Paris
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Argonne National Laboratory, 9700 South Cass Avenue
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Department of Physics Duke University
Center for Cosmology and Astro-Particle Physics The Ohio State University
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Department of Physics The Ohio State University
Santa Cruz Institute for Particle Physics
Jet Propulsion Laboratory California Institute of Technology, 4800 Oak Grove Dr.
Faculty of Physics Ludwig-Maximilians-Universitat, Scheinerstr. 1
Department of Physics University of Oxford Denys Wilkinson Building, Keble Road
Jodrell Bank Center for Astrophysics School of Physics and Astronomy University of Manchester, Oxford Road
Department of Physics University of Michigan
Department of Applied Mathematics and Theoretical Physics University of Cambridge
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Institut d'Estudis Espacials de Catalunya (IEEC)
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Sorbonne Universites Upmc Univ Paris 06 Umr 7095 Institut d'Astrophysique de Paris
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Institute for Fundamental Physics of the Universe, Via Beirut 2
Observatorio Nacional, Rua Gal. José Cristino 77, RJ
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School of Mathematics and Physics University of Queensland
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Department of Physics Iit Hyderabad, Telangana
Department of Astronomy University of Michigan
Institute of Theoretical Astrophysics University of Oslo, P.O. Box 1029 Blindern
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Australian Astronomical Optics Macquarie University
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