Measurements of large-scale structure are interpreted using theoretical predictions for the matter distribution, including potential impacts of baryonic physics...
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PublicationDark energy survey year 1 results: Constraining baryonic physics in the Universe
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PublicationDark energy survey year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
We present cosmological constraints from the analysis of angular power spectra of cosmic shear maps based on data from the first three years of observations by...
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PublicationDark Energy Survey Year 3 results: galaxy clustering and systematics treatment for lens galaxy samples
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a magnitude-limited sample optimized for the measurement of...
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PublicationDark Energy Survey Year 3 results: magnification modelling and impact on cosmological constraints from galaxy clustering and galaxy-galaxy lensing
We study the effect of magnification in the Dark Energy Survey Year 3 analysis of galaxy clustering and galaxy-galaxy lensing, using two different lens samples...
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PublicationDark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
We use a combination of three large N-body simulations to investigate the dependence of dark matter halo concentrations on halo mass and redshift in the...
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PublicationDensity weighted angular redshift fluctuations: a new cosmological observable
We propose the use of angular fluctuations in the galaxy redshift field as a new way to extract cosmological information in the Universe. This new probe $\delta...
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PublicationDES Y3 cosmic shear down to small scales: Constraints on cosmology and baryons
We present the first analysis of cosmic shear measured in DES Y3 that employs the entire range of angular scales in the data. To achieve this, we built upon...
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PublicationErratum: A modified χ2-test for cosmic microwave background analyses
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PublicationErratum: Dark matter halo concentrations in the Wilkinson Microwave Anisotropy Probe year 5 cosmology
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