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Implicit Priors in Galaxy Cluster Mass and Scaling Relation Determinations

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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Importance of far-infrared mapping in a spiral galaxy: AKARI observation of M81

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Imprint of Accretion Disk-Induced Migration on Gravitational Waves from Extreme Mass Ratio Inspirals

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Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence

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Imprints of a hemispherical power asymmetry in the seven-year WMAP data due to non-commutativity of space-time

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Imprints of anisotropic inflation on the cosmic microwave background

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Imprints of Dark Energy on Cosmic Structure Formation I) Realistic Quintessence Models and the Non-Linear Matter Power Spectrum

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Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function

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Imprints of dynamical dark energy on weak-lensing measurements

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Imprints of primordial non-Gaussianities in X-ray and SZ signals from galaxy clusters

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Imprints of primordial non-Gaussianity on the number counts of cosmic shear peaks

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Imprints of the QCD Phase Transition on the Spectrum of Gravitational Waves

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Improved and Quality-assessed Emission and Absorption Line measurements in Sloan Digital Sky Survey galaxies

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Improved CMB Map from WMAP Data

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Improved collision strengths and line ratios for forbidden [O III] far-infrared and optical lines

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Improved composite spectra of quasars within the HI Lyα-forest region

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Improved constraints on cosmic microwave background secondary anisotropies from the complete 2008 South Pole Telescope data

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Improved constraints on cosmological parameters from SNIa data

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Improved Constraints on Inelastic Dark Matter

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Improved constraints on primordial non-Gaussianity for the Wilkinson Microwave Anisotropy Probe 5-yr data

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