1.     Observational tests of gravity and dark energy

2.     Ultra-large scales and future experiments (Euclid and the SKA)

3.     Kinetic field theory of large-scale structure and nonlinear observables

4.     Local tests of gravity

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1.     Inflation and primordial anisotropies

2.     The  role of defects during inflation

3.     The application of “delta N” formalism in anisotropic backgrounds

4.     EFT approach to anisotropic inflation

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1.     Random fields in cosmology (random fields, central limit theorem, cosmic structure formation, fluid mechanics, linearization, nonlinearities and non-Gaussianities)

2.     Statistical inference in cosmology (likelihoods, Bayesian statistics, statistical errors and the Fisher-formalism, Systematic errors, MCMC techniques, model selection, statistical evidence)

3.     Squeezing cosmological information out of a weak lensing survey  

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1.       Standard model of cosmology

2.       Current status and the future of observational cosmology from CMB to LSS.

3.       CMB after Planck (theory, experiments and their scientific goals)   

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1.       Effective field theory in cosmology

2.       Precision comparison of the Power Spectrum in the EFT of LSS

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1.     Special topics in data analysis in cosmology

2.     Beyond the standard model of cosmology

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1.     Structure formation:  Linear theory, P(k) and the BAO

2.     The excursion set approach:  Halo abundances and clustering

3.     The Halo Model in practice

4.     The BAO linear point: A cleaner cosmological standard ruler

5.     Assembly bias:  Halo stochasticity and the cosmic web

6.     Non-Markovian random walks

7.     Mark correlation functions

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1.       Introduction to Inflation and primordial observables

2.       B modes, large fields, and axion monodromy

3.       Non-Gaussianity and QFT (new results)

4.       Different approaches to inflation in string theory

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