Future cosmology with CMB lensing and galaxy clustering Prospects for CMB lensing-galaxy clustering cross-correlations and modeling biased tracers Modeling biased tracers at the field level Extracting linear information from
nonlinear large-scale structure observations Prospects for CMB lensing-galaxy clustering cross-correlations and initial condition reconstruction Large-Scale Structure beyond the Power Spectrum Large-scale structure non-Gaussianities with modal methods (Ascona) Joint analysis of CMB temperature and lensing-reconstruction power spectra