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Stefan Hilbert (LMU)18/10/2016, 09:30Welcome, practical information, and outline of workshopGo to contribution page
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Stefan Hilbert (LMU)18/10/2016, 10:00topical introduction to workshopGo to contribution page
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Dr Joachim Stadel (University of Zurich)18/10/2016, 11:00I will discuss the method employed in our recent 2 trillion particle simulation for generating a light cone where the look-back time and comoving distance from the observer is an exact linear function for every particle. While such an approach may seem to be extremely costly at face value, it turns out to be quite efficient for reasonably large cosmological volumes. I will also discuss...Go to contribution page
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Mr Sownak Bose (Institute for Computational Cosmology)18/10/2016, 11:30We present a ray tracing code to compute integrated cosmological observables on the fly in AMR N-body simulations. Unlike conventional ray tracing techniques, this code takes full advantage of the time and spatial resolution attained by the N-body simulation by computing the integrals along the line of sight on a cell-by-cell basis through the AMR simulation grid. Moreover, since it runs on...Go to contribution page
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Dr Claudio Llinares (Durham University)18/10/2016, 12:00While doing predictions for gravitational lensing using first order equations greatly simplifies the calculations, it has been shown that the approximations involved can not reach the accuracy required by the next generation of galaxy surveys. Second order effects must be included in lensing predictions. Since this is new territory, it is important that we do not focus only on one technique,...Go to contribution page
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Mr Alexander Smith (Durham University)18/10/2016, 14:00With upcoming galaxy surveys, such as DESI and Euclid, it is important to have realistic mock catalogues which can be used, for example, to test methods of measuring statistics from the survey and removing systematic effects. For this purpose, we have created a full sky mock catalogue that is complete to r=20 from the Millennium-XXL (MXXL) simulation. We have generated a MXXL halo lightcone...Go to contribution page
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Dr Francisco Javier Castander (ICE, IEEC-CSIC)18/10/2016, 14:30We will summarize the MICE simulations and the way we have built a lightcone in the dark matter distribution and for the lensing observablesGo to contribution page
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Dr Katarina Markovic (ICG Portsmouth)18/10/2016, 15:00
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18/10/2016, 16:00
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Dr Carmelita Carbone (INAF - Milan)19/10/2016, 09:00I discuss Born and post-Born full-sky lensing ray-tracing in N-Body simulations.Go to contribution page
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Dr Jens Jasche (TUM)19/10/2016, 09:45Next generation cosmological surveys will provide an avalanche of cosmological observations. This increase in scientific data needs to be accompanied with the development of novel information processing techniques to interpret such observations. Analyses of three dimensional inhomogeneous large scale structures require to jointly account for complex dynamical processes, associated to the...Go to contribution page
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Dr Carlo Giocoli (Department of Physics and Astronomy - Alma Mater Studiorum UniBO)19/10/2016, 11:00
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Emiliano Munari (INAF Osservatorio Astronomico Trieste)19/10/2016, 11:45Pinocchio is a tool to generate in an approximate but fast way catalogs of DM halos. The new version comes with on-the-fly production of halo catalog on the past light cone with continuous time sampling.Go to contribution page
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Dr Santiago Avila (Institute of Cosmology and Gravitation)19/10/2016, 14:00
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Mr Rodríguez-Torres Sergio (Instituto de Física Teórica/Departamento de Física Teórica UAM/CSIC)19/10/2016, 14:30
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Dr Katarina Markovic (ICG Portsmouth)19/10/2016, 15:00
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19/10/2016, 16:00
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Dr Dylan Nelson (MPA)20/10/2016, 10:00
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20/10/2016, 11:00
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Stefan Hilbert (LMU)20/10/2016, 14:00
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Stefan Hilbert (LMU)20/10/2016, 15:00
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