Cosmic Microwave Background Radiation

Cosmological parameters 2006

Galaxy Clusters / Power Spectrum / Cosmic Microwave Background Radiation / Scale Invariance / Perturbation Theory

THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGICAL PARAMETERS FROM THE 2008 POWER SPECTRUM

Organic Chemistry / Astrophysical Plasma / Kinetics / Parameter estimation / Cosmic Microwave Background / Seasonality / Spectrum / Infrared / Power Spectrum / Analytical Model / Indexation / Cosmic Microwave Background Radiation / Cosmic String / Scale Invariance / Seasonality / Spectrum / Infrared / Power Spectrum / Analytical Model / Indexation / Cosmic Microwave Background Radiation / Cosmic String / Scale Invariance

The Atacama Cosmology Telescope: Cosmological Parameters From the 2008 Power Spectrum

Organic Chemistry / Astrophysical Plasma / Kinetics / Parameter estimation / Cosmic Microwave Background / Seasonality / Subject headings / Spectrum / Infrared / Power Spectrum / Analytical Model / Indexation / Cosmic Microwave Background Radiation / Cosmic String / Scale Invariance / Seasonality / Subject headings / Spectrum / Infrared / Power Spectrum / Analytical Model / Indexation / Cosmic Microwave Background Radiation / Cosmic String / Scale Invariance

Primordial spectrum and density parameter-problem in a power-law inflation

Dark Matter / Dust (Astronomy & Astrophysics) / Big Bang / Open University / Power Law / Spectral method / Spectrum / Cold Dark Matter / Binding Energy / Exponential Growth / Background Radiation / Boolean Satisfiability / Large Scale / Cosmic Microwave Background Radiation / Scale Invariance / Spectral method / Spectrum / Cold Dark Matter / Binding Energy / Exponential Growth / Background Radiation / Boolean Satisfiability / Large Scale / Cosmic Microwave Background Radiation / Scale Invariance

Primordial spectrum and density parameter-problem in a power-law inflation

Dark Matter / Dust (Astronomy & Astrophysics) / Big Bang / Open University / Power Law / Spectral method / Spectrum / Cold Dark Matter / Binding Energy / Exponential Growth / Background Radiation / Boolean Satisfiability / Large Scale / Cosmic Microwave Background Radiation / Scale Invariance / Spectral method / Spectrum / Cold Dark Matter / Binding Energy / Exponential Growth / Background Radiation / Boolean Satisfiability / Large Scale / Cosmic Microwave Background Radiation / Scale Invariance

Primordial spectrum and density parameter-problem in a power-law inflation

Dark Matter / Dust (Astronomy & Astrophysics) / Big Bang / Open University / Power Law / Spectral method / Spectrum / Cold Dark Matter / Binding Energy / Exponential Growth / Background Radiation / Boolean Satisfiability / Large Scale / Cosmic Microwave Background Radiation / Scale Invariance / Spectral method / Spectrum / Cold Dark Matter / Binding Energy / Exponential Growth / Background Radiation / Boolean Satisfiability / Large Scale / Cosmic Microwave Background Radiation / Scale Invariance

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