Por favor, use este identificador para citar o enlazar a este item:
http://hdl.handle.net/10261/296605
COMPARTIR / EXPORTAR:
SHARE CORE BASE | |
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE | |
Título: | Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. I. Measurements, systematics tests, and feedback model constraints |
Autor: | Gatti, M.; Pandey, Shiwam; Crocce, Martín CSIC ORCID; Fosalba, Pablo CSIC ORCID; García-Bellido, Juan CSIC ORCID; Gaztañaga, Enrique CSIC ORCID; Serrano, Sergio; DES and ACT Collaboration | Fecha de publicación: | 2022 | Editor: | American Physical Society | Citación: | Physical Review D 105(12): 123525 (2022) | Resumen: | We present a tomographic measurement of the cross-correlation between thermal Sunyaev-Zel’dovich (TSZ) maps from Planck and the Atacama Cosmology Telescope and weak galaxy lensing shears measured during the first three years of observations of the Dark Energy Survey. This correlation is sensitive to the thermal energy in baryons over a wide redshift range and is therefore a powerful probe of astrophysical feedback. We detect the correlation at a statistical significance of 21σ, the highest significance to date. We examine the TSZ maps for potential contaminants, including cosmic infrared background and radio sources, finding that cosmic infrared background has a substantial impact on our measurements and must be taken into account in our analysis. We use the cross-correlation measurements to test different feedback models. In particular, we model the TSZ using several different pressure profile models calibrated against hydrodynamical simulations. Our analysis marginalizes over redshift uncertainties, shear calibration biases, and intrinsic alignment effects. We also marginalize over Ωm and σ8 using Planck or DES priors. We find that the data prefer the model with a low amplitude of the pressure profile at small scales, compatible with a scenario with strong active galactic nuclei feedback and ejection of gas from the inner part of the halos. When using a more flexible model for the shear profile, constraints are weaker, and the data cannot discriminate between different baryonic prescriptions. | Descripción: | DES and ACT Collaboration: M. Gatti et al. | Versión del editor: | https://doi.org/10.1103/PhysRevD.105.123525 | URI: | http://hdl.handle.net/10261/296605 | DOI: | 10.1103/PhysRevD.105.123525 | E-ISSN: | 2470-0029 |
Aparece en las colecciones: | (ICE) Artículos (IFT) Artículos |
Ficheros en este ítem:
Fichero | Descripción | Tamaño | Formato | |
---|---|---|---|---|
crossconstra.pdf | 3,36 MB | Adobe PDF | Visualizar/Abrir |
CORE Recommender
SCOPUSTM
Citations
16
checked on 17-abr-2024
WEB OF SCIENCETM
Citations
8
checked on 25-feb-2024
Page view(s)
18
checked on 24-abr-2024
Download(s)
31
checked on 24-abr-2024
Google ScholarTM
Check
Altmetric
Altmetric
NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.