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Testing General Relativity on Horizon Scales and the Primordial non-Gaussianity

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Testing General Relativity using the Environmental Dependence of Dark Matter Halos

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Testing General Relativity with Current Cosmological Data

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Testing generic predictions of dark energy

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Testing gravity on kiloparsec scales with strong gravitational lenses

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Testing gravity using the growth of large scale structure in the Universe

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Testing gravity with CAMB and CosmoMC

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Testing gravity with halo density profiles observed through gravitational lensing

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Testing Gravity with the Stacked Phase Space around Galaxy Clusters

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Testing homogeneity with galaxy number counts : light-cone metric and general low-redshift expansion for a central observer in a matter dominated isotropic universe without cosmological constant

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Testing homogeneity with the fossil record of galaxies

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Testing Inflation with Dark Matter Halos

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Testing inflationary consistency relations by the potential CMB observations

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Testing large-angle deviation from Gaussianity in CMB maps

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Testing Local Lorentz Invariance with high-accuracy astrometric observations

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Testing Lorentz Invariance with Neutrinos from Ultrahigh Energy Cosmic Ray Interactions

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Testing model independent modified gravity with future large scale surveys

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Testing models for molecular gas formation in galaxies: hydrostatic pressure or gas and dust shielding?

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Testing modified gravity models with recent cosmological observations

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Testing Modified Newtonian Dynamics with Rotation Curves of Dwarf and Low Surface Brightness Galaxies

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