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Francesco Montanari

Researcher at Autonomous University of Madrid

Publications -  15
Citations -  710

Francesco Montanari is an academic researcher from Autonomous University of Madrid. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 11, co-authored 15 publications receiving 513 citations. Previous affiliations of Francesco Montanari include University of Geneva & Helsinki Institute of Physics.

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Galileon Gravity in Light of ISW, CMB, BAO and $H_0$ data

TL;DR: In this paper, the authors place constraints on the full parameter space of these models using data from the cosmic microwave background (CMB) (including lensing), baryonic acoustic oscillations (BAO) and the Integrated Sachs-Wolfe (ISW) effect.

Cosmology and Fundamental Physics with the Euclid Satellite

TL;DR: This review is meant to provide a guide to the scientific themes that will underlie the activity of the group during the preparation of the Euclid mission and discusses five broad topics: dark energy and modified gravity, dark matter, initial conditions, basic assumptions and questions of methodology in the data analysis.
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Cosmological Measurements with General Relativistic Galaxy Correlations

TL;DR: In this article, the cosmological dependence and the constraining power of large-scale galaxy correlations, including all redshift-distortions, wide-angle, lensing and gravitational potential effects on linear scales, are investigated.
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Lensing convergence and the neutrino mass scale in galaxy redshift surveys

TL;DR: In this article, the importance of including the lensing contribution in galaxy clustering analyses with large galaxy redshift surveys is demonstrated. But neglecting lensing in the autocorrelations within one bin severely biases cosmological parameter estimation.
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Model-Independent Determination of H 0 and Ω K 0 from Strong Lensing and Type Ia Supernovae

TL;DR: The first determination of the Hubble constant H_{0} is presented from strong lensing time delay data and type Ia supernova luminosity distances and the spatial curvature model is determined independently.