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Large-scale galaxy bias
This review presents a comprehensive overview of galaxy bias, that is, the statistical relation
between the distribution of galaxies and matter. We focus on large scales where cosmic …
between the distribution of galaxies and matter. We focus on large scales where cosmic …
Weak lensing for precision cosmology
R Mandelbaum - Annual Review of Astronomy and Astrophysics, 2018 - annualreviews.org
Weak gravitational lensing, the deflection of light by mass, is one of the best tools to
constrain the growth of cosmic structure with time and reveal the nature of dark energy. I …
constrain the growth of cosmic structure with time and reveal the nature of dark energy. I …
Measurement of parity-odd modes in the large-scale 4-point correlation function of Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey twelfth data …
ABSTRACT A tetrahedron is the simplest shape that cannot be rotated into its mirror image
in three-dimension (3D). The 4-point correlation function (4PCF), which quantifies excess …
in three-dimension (3D). The 4-point correlation function (4PCF), which quantifies excess …
Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
We measure cosmic weak lensing shear power spectra with the Subaru Hyper Suprime-
Cam (HSC) survey first-year shear catalog covering 137 deg2 of the sky. Thanks to the high …
Cam (HSC) survey first-year shear catalog covering 137 deg2 of the sky. Thanks to the high …
The quijote simulations
The Quijote Simulations - IOPscience Skip to content IOP Science home Accessibility Help
Search all IOPscience content Search Article Lookup Select journal (required) Volume …
Search all IOPscience content Search Article Lookup Select journal (required) Volume …
KiDS-450: cosmological parameter constraints from tomographic weak gravitational lensing
H Hildebrandt, M Viola, C Heymans… - Monthly Notices of …, 2017 - academic.oup.com
We present cosmological parameter constraints from a tomographic weak gravitational
lensing analysis of∼ 450 deg2 of imaging data from the Kilo Degree Survey (KiDS). For a …
lensing analysis of∼ 450 deg2 of imaging data from the Kilo Degree Survey (KiDS). For a …
Cosmology with cosmic shear observations: a review
M Kilbinger - Reports on Progress in Physics, 2015 - iopscience.iop.org
Cosmic shear is the distortion of images of distant galaxies due to weak gravitational lensing
by the large-scale structure in the Universe. Such images are coherently deformed by the …
by the large-scale structure in the Universe. Such images are coherently deformed by the …
KiDS-1000 methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
We present the methodology for a joint cosmological analysis of weak gravitational lensing
from the fourth data release of the ESO Kilo-Degree Survey (KiDS-1000) and galaxy …
from the fourth data release of the ESO Kilo-Degree Survey (KiDS-1000) and galaxy …
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
FS Kitaura, S Rodriguez-Torres… - Monthly Notices of …, 2016 - academic.oup.com
We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation
Spectroscopic Survey Final Data Release (BOSS DR11&DR12) with high fidelity on all …
Spectroscopic Survey Final Data Release (BOSS DR11&DR12) with high fidelity on all …
Large-scale dark matter simulations
We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …
Universe. We start by providing the main set of equations solved by these simulations and …