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Testing general relativity in cosmology
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The clustering of massive Primordial Black Holes as Dark Matter: Measuring their mass distribution with advanced LIGO
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On simple analytic models of microlensing amplification statistics
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Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies
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Observational evidence for primordial black holes: A positivist perspective
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Uncovering a population of gravitational lens galaxies with magnified standard candle SN Zwicky
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Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
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Planck 2018 results: VI. Cosmological parameters
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A hydrodynamical halo model for weak-lensing cross correlations
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An analytical approach to gravitational lensing by an ensemble of axisymmetric lenses
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Gravitational microlensing of high-redshift supernovae by compact objects
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June 1991 |
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April 1992 |
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On the probability of magnification by cosmologically distributed gravitational lenses
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January 1993 |
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The Distance-Redshift Relation for Universes with no Intergalactic Medium
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June 1972 |
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The Effects of Inhomogeneities on Evaluating the Mass Parameter Ωmand the Cosmological Constant Λ
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Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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June 1999 |
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A Fundamental Test of the Nature of Dark Matter
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July 1999 |
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A Universal Probability Distribution Function for Weak-lensing Amplification
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June 2002 |
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Safety in Numbers: Gravitational Lensing Degradation of the Luminosity Distance–Redshift Relation
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Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies
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September 2009 |
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Revising the Halofit Model for the Nonlinear Matter Power Spectrum
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The Effect of weak Lensing on Distance Estimates from Supernovae
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Constraints on primordial black holes
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New X-ray bound on density of primordial black holes
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Accurate modelling of extragalactic microlensing by compact objects
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On the Possibility of Determining Hubble's Parameter and the Masses of Galaxies from the Gravitational Lens Effect
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Weak lensing of Type Ia Supernovae from the Dark Energy Survey
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1
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September 2020 |
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the quasar sample in configuration space between redshift 0.8 and 2.2
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October 2020 |
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
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December 2020 |
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Dark Energy Survey Year 3 results: Curved-sky weak lensing mass map reconstruction
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May 2021 |
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The dark energy survey 5-yr photometrically identified type Ia supernovae
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Weak-lensing magnification of Type Ia supernovae from the Pantheon sample
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June 2022 |
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A galaxy-driven model of type Ia supernova luminosity variations
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July 2022 |
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A non-linear solution to the S8 tension?
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September 2022 |
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Strong lensing constraints on primordial black holes as a dark matter candidate
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May 2023 |
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Type Ia supernova constraints on compact object dark matter
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The dark energy survey: detection of weak lensing magnification of supernovae and constraints on dark matter haloes
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The dark energy survey supernova program: investigating beyond-ΛCDM
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The abundance of dark matter haloes down to Earth mass
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An algorithm to build mock galaxy catalogues using MICE simulations
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December 2014 |
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The MICE Grand Challenge light-cone simulation – III. Galaxy lensing mocks from all-sky lensing maps
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The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15
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March 2015 |
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The MICE Grand Challenge lightcone simulation – II. Halo and galaxy catalogues
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August 2015 |
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polychord: next-generation nested sampling
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On the bias of the distance–redshift relation from gravitational lensing
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December 2015 |
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Testing the lognormality of the galaxy and weak lensing convergence distributions from Dark Energy Survey maps
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August 2016 |
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
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Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory
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April 2021 |
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January 2022 |
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Dark Energy Survey Year 3 results: Constraints on extensions to ΛCDM with weak lensing and galaxy clustering
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