Euclid preparation. TBD. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid
Tue, 13/02/2024 - 14:06
mchane-y
arXiv e-prints. p. arXiv:2310.15731, 2023.
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Cosmologie et eXtragalactique
Direct Optimal Mapping Image Power Spectrum and its Window Functions
Tue, 13/02/2024 - 14:05
mchane-y
arXiv e-prints. p. arXiv:2311.10711, 2023.
Inferring reionization and galaxy properties from the patchy kinetic Sunyaev-Zel'dovich signal
Tue, 13/02/2024 - 14:05
mchane-y
Monthly Notices of the RAS, vol. 526. pp. 3170-3183, 2023.
Constraining cosmic reionization by combining the kinetic Sunyaev-Zel'dovich and the 21 cm power spectra
Tue, 13/02/2024 - 14:03
mchane-y
arXiv e-prints. p. arXiv:2312.04259, 2023.
matvis: A matrix-based visibility simulator for fast forward modelling of many-element 21 cm arrays
Tue, 13/02/2024 - 14:02
mchane-y
arXiv e-prints. p. arXiv:2312.09763, 2023.
matvis: Fast matrix-based visibility simulator
Tue, 13/02/2024 - 14:02
mchane-y
2023.
Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning
Tue, 13/02/2024 - 14:01
mchane-y
arXiv e-prints. p. arXiv:2401.04304, 2024.
French
BATMAN is an ANR funded project aiming at providing better accuracy and robustness of the neutrino mass assessment from CMB experiments. Experts in CMB data and likelihood, reionisation history and gas physics, distributed in three nodes (IAS-Orsay, IJClab-Orsay, IRAP-Toulouse) will work on the project for the 3 years duration of the project.
Illustration du projet:
English
LOCALIZATION (LOcal Clusters And superclusters in sZ: Adding Thermal, kinetic and relativistic cOrrectioNs) is project funded by ANR international aiming at producing constrained hydrodynamical simulations in order to investigate the cosmological imprints of galaxy clusters and the local Universe.
Principal Investigator: Nabila Aghanim
Illustration du projet:
French
LOCALIZATION (LOcal Clusters And superclusters in sZ: Adding Thermal, kinetic and relativistic cOrrectioNs) est un projet ANR internationale visant à produire des simulations hydrodynamiques contraintes pour étudier les signatures cosmologiques des amas de galaxies et de l'Univers local.
Principal Investigator: Nabila Aghanim
Illustration du projet:
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