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Matter power spectrum
THE NONLINEAR MATTER POWER SPECTRUM1 Online Material
Planck Early Results. XVIII. the Power Spectrum of Cosmic Infrared Background Anisotropies
Clusters, Cosmology and Reionization from the SZ Power Spectrum
Cosmological Structure Formation with Modified Gravity
The Effects of the Small-Scale Behaviour of Dark Matter Power Spectrum on CMB Spectral Distortion
Year 1 Cosmology Results from the Dark Energy Survey
Cosmology from Cosmic Shear and Robustness to Data Calibration
Cosmic Microwave Background
6 Structure Formation – I
Dark Energy Survey Year 3 Results: Multi-Probe Modeling Strategy and Validation
Retrieving the Three-Dimensional Matter Power Spectrum and Galaxy Biasing Parameters from Lensing Tomography
Bias in Matter Power Spectra?
On Dark Matter - Dark Radiation Interaction and Cosmic Reionization
Nonparametric Inference for the Cosmic Microwave Background Christopher R
Imprints of the Early Universe on Axion Dark Matter Substructure
Modeling the Power Spectrum in High-Redshift Galaxy Surveys
Steps Toward the Power Spectrum of Matter. III. the Primordial Spectrum
Origin and Evolution of the Universe CMB and Structure Formation
Top View
Observational Cosmology: Large Scale Structure
Mixed Dark Matter: Matter Power Spectrum and Halo Mass Function
Full List of COSMOIGM Publications
The Power Spectrum and the Matter Content of the Universe
Cosmological Constraints from Cosmic Shear
Particle Astrophysics and Cosmology: Cosmic Laboratories for New Physics (Summary of the Snowmass 2001 P4 Working Group)
Arxiv:2011.15018V1 [Astro-Ph.CO] 30 Nov 2020 Particle
The Dark Energy Survey♣
Testing (Modified) Gravity with 3D and Tomographic Cosmic Shear
Matter Power Spectrum and the Challenge of Percent Accuracy
Structure Formation Risa Wechsler
Understanding the CMB Temperature Power Spectrum
Cosmological Constraints from Galaxy Clustering and Weak Lensing
Part-III Cosmology Michaelmas Term 2009
Secondary Signals in Cosmology
Cosmology from Secondary Anisotropies of the Cosmic Microwave Background
Analytic Model for the Matter Power Spectrum, Its Covariance Matrix and Baryonic Effects
24. Cosmological Parameters 1 24
From Microwave Anisotropies to Cosmology
Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
CMB Polarization and Cosmology
The Mildly Non-Linear Regime of Structure Formation
The CMB, Dark Matter and Dark Energy
Arxiv:2103.01229V2 [Astro-Ph.CO] 25 May 2021 Contents
Simulating Structure Formation in SIDM
Euclid Imaging Consortium Science Book
Projection Effects on the Observed Angular Spectrum of the Astrophysical Stochastic Gravitational Wave Background
Galaxy Clustering in Redshift Space
Probing Self-Interacting Dark Matter Via Matter Power Spectrum
Revisiting the Post-Reionization Kinetic Sunyaev-Zel'dovich Effect
Arxiv:2011.07722V2 [Astro-Ph.CO] 21 Jan 2021
Cosmological Observations in a Modified Theory of Gravity
The Matter Power Spectrum in Redshift Space Using Effective Field Theory
The Effects of Galaxy Formation on the Matter Power Spectrum
Contribution of Non-Linear Structure to the Kinetic Sunyaev-Zeldovich Power Spectrum
Non-Linear Contributions to Angular Power Spectra
Position-Dependent Power Spectra of the 21-Cm Signal from the Epoch of Reionization
The Matter Power Spectrum
Response Approach to the Matter Power Spectrum Covariance
Cosmic Microwave Background 1 26
The Dark Energy Survey Science Program
Lyman-Α Power Spectrum As a Probe of Modified Gravity
Accepted Manuscript
Non-Linear Evolution of Cosmological Power-Spectra Using the Kinetic Field Theory Approach
Quantifying Baryon Effects on the Matter Power Spectrum and the Weak Lensing Shear Correlation
Arxiv:2007.00555V2 [Astro-Ph.CO] 19 Oct 2020 Batic: Overdense Regions Have an Excess of Baryons, Dark Satisfactory Alternative to General Relativity (GR)
An Introduction to Cosmology
Also-Read Query Results
General Requirements on Matter Power Spectrum Predictions for Cosmology with Weak Lensing Tomography Arxiv:1111.0052V2 [Astro-P
14.1 Overview