MS

Marcel Schmittfull

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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