Cosmological Research at ITA
Gravitational Lensing
- Strong lensing by galaxy clusters
- formation of arcs in galaxy clusters
- statistics of arcs and cosmological implications
- diagnostics of galaxy clusters using arcs
- Weak lensing by galaxy clusters
- detection of dark-matter halos using weak lensing
- dependence of weak lensing on mass profiles
- cosmological implications of weak lensing
- statistics of weak-lensing effects
- Strong lensing by galaxies
- effects of spiral disks on multiple imaging
Galaxy Clusters
- Hot gas in galaxy clusters
- diagnostics of clusters from their X-ray emission
- thermal and kinetic Sunyaev-Zel'dovich effects
- joint cluster analyses using multi-band data
- Magnetic fields in galaxy clusters
- origin and evolution of cluster magnetic fields
- non-thermal emission due to magnetic fields
- Faraday rotation
Cosmology
- Structure formation
- growth of dark-matter halos in different cosmological models
- diagnostics for halo properties
- Dark matter and dark energy
- matter distribution in dark halos
- implications of dark energy for structure growth
- observational consequences of dark-energy models
- Cosmic microwave background (CMB)
- Gravitational lensing of the CMB
- Secondary anisotropies and source detection
Planck Project
- software and algorithm development for the Planck satellite
- data centre for Planck at MPA
- scientific exploitation of Planck data
Responsible: Matthias Bartelmann, last modification Wednesday, 16-May-2007 09:45:39 CEST