Séminaire Univers / |
| « Forward modelling large scale tracers of initial conditions » |
|
George Stein |
| Large scale structure simulations are required for a large number of problems in cosmology. When huge ensembles of mock halo catalogues are needed, traditional N-body methods are not fast enough. I will discuss a CITA led effort to use “approximate” methods, such as the Peak Patch approach, to develop mocks for next generation future surveys such as Euclid, CMB-s4, and COMAP. |
|
jeudi 19 octobre 2017 - 15:00 Salle 281 Institut d'Astrophysique de Paris |
| Pages web du séminaire / Seminar's webpage |