Large-scale structure of the Universe and cosmological perturbation theory
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September 2002 |
Large-scale galaxy bias
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February 2018 |
Second-order power spectrum and nonlinear evolution at high redshift
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August 1994 |
Coupling of modes of cosmological mass density fluctuations
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December 1986 |
Resumming cosmological perturbations via the Lagrangian picture: One-loop results in real space and in redshift space
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March 2008 |
Renormalized cosmological perturbation theory
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March 2006 |
The effective field theory of cosmological large scale structures
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September 2012 |
A Lagrangian effective field theory
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September 2015 |
Biasing and hierarchical statistics in large-scale structure
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August 1993 |
Galaxy formation with a local bias
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June 1993 |
The non-linear redshift-space power spectrum of galaxies
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December 1998 |
Constraints on the Effects of Locally Biased Galaxy Formation
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September 1998 |
Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
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August 2009 |
Integrated perturbation theory and one-loop power spectra of biased tracers
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August 2014 |
Convolution Lagrangian perturbation theory for biased tracers
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December 2012 |
The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9: WiggleZ Survey: growth of structure
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June 2011 |
The WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with three-point correlation functions
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May 2013 |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges
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September 2016 |
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
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October 2016 |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space
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December 2016 |
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample
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January 2017 |
The cosmological analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
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May 2020 |
Cosmological parameters and neutrino masses from the final P l a n c k and full-shape BOSS data
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April 2020 |
Halo models of large scale structure
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December 2002 |
The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and Mass
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August 2002 |
Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
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November 2005 |
Galaxy–galaxy lensing in the Dark Energy Survey Science Verification data
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November 2016 |
The Luminosity and Color Dependence of the Galaxy Correlation Function
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September 2005 |
Understanding higher-order nonlocal halo bias at large scales by combining the power spectrum with the bispectrum
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December 2014 |
On the statistics of biased tracers in the Effective Field Theory of Large Scale Structures
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September 2015 |
Impact of bias and redshift-space modelling for the halo power spectrum: testing the effective field theory of large-scale structure
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July 2020 |
Renormalization of linear halo bias in N-body simulations
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December 2019 |
Testing one-loop galaxy bias: Power spectrum
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November 2020 |
Stochasticity of Bias and Nonlocality of Galaxy Formation: Linear Scales
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November 1999 |
Stochastic Nonlinear Galaxy Biasing
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July 1999 |
Stochastic Biasing and the Galaxy–Mass Density Relation in the Weakly Nonlinear Regime
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September 1999 |
Gravity and large-scale nonlocal bias
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April 2012 |
The Evolution of Bias
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April 1996 |
Evidence for quadratic tidal tensor bias from the halo bispectrum
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October 2012 |
Halo bias in Lagrangian space: estimators and theoretical predictions
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August 2017 |
Cosmological constraints from a combination of galaxy clustering and lensing – I. Theoretical framework
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journal
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February 2013 |
Controlling and leveraging small-scale information in tomographic galaxy–galaxy lensing
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October 2019 |
Algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering
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March 2010 |
The dark Energy Camera
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October 2015 |
The Dark Energy Survey Image Processing Pipeline
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May 2018 |
The cosmological simulation code gadget-2
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December 2005 |
The MICE grand challenge lightcone simulation – I. Dark matter clustering
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March 2015 |
An algorithm to build mock galaxy catalogues using MICE simulations
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December 2014 |
The MICE Grand Challenge lightcone simulation – II. Halo and galaxy catalogues
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journal
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August 2015 |
redMaGiC: selecting luminous red galaxies from the DES Science Verification data
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May 2016 |
Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
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August 2018 |
DES Y1 Results: validating cosmological parameter estimation using simulated Dark Energy Surveys
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July 2018 |
Effective field theory of gravity for extended objects
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May 2006 |
Bias in the effective field theory of large scale structures
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November 2015 |
Cosmological non-linearities as an effective fluid
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July 2012 |
Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
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November 2019 |
Revising the Halofit Model for the Nonlinear Matter Power Spectrum
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December 2012 |
Effective field theory of large scale structure at two loops: The apparent scale dependence of the speed of sound
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December 2015 |
FAST-PT: a novel algorithm to calculate convolution integrals in cosmological perturbation theory
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September 2016 |
FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory
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February 2017 |
Fast large scale structure perturbation theory using one-dimensional fast Fourier transforms
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May 2016 |
Notes on bias in Estimation
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January 1956 |
Abstracts of Papers
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June 1958 |
Statistical analysis of galaxy surveys - I. Robust error estimation for two-point clustering statistics
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June 2009 |
Performance of internal covariance estimators for cosmic shear correlation functions
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December 2015 |
Why your model parameter confidences might be too optimistic. Unbiased estimation of the inverse covariance matrix
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December 2006 |
Bias and variance of angular correlation functions
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July 1993 |
The skewness of the aperture mass statistic
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July 2004 |
CosmoSIS: Modular cosmological parameter estimation
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September 2015 |