Bruno Moraes

Dispersion of growth of matter perturbations in f ( R ) gravity

We study the growth of matter density perturbations

First measurement of the cross-correlation of CMB lensing and galaxy lensing

{\ensuremath{\delta}}_{m}

Chameleon dark energy models with characteristic signatures

for a number of viable

Lensing is Low: Cosmology, Galaxy Formation, or New Physics?

f(R)

Cosmological constraints from weak lensing peak statistics with Canada-France-Hawaii Telescope Stripe 82 Survey

gravity models that satisfy both cosmological and local gravity constraints, where the Lagrangian density

Weak lensing mass map and peak statistics in Canada–France–Hawaii Telescope Stripe 82 survey

f

First galaxy–galaxy lensing measurement of satellite halo mass in the CFHT Stripe-82 Survey

is a function of the Ricci scalar

Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis

R

Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey

. If the parameter

The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey

m\ensuremath{\equiv}R{f}_{,RR}/{f}_{,R}