Patrick Stoecker
(Institute for Theoretical Particle Physics and Cosmology, RWTH Aachen)
04/11/2020, 09:00
Cyril Pitrou
(Institut d'Astrophysique de Paris)
04/11/2020, 09:40
Deanna C. Hooper
(ULB (Université libre de Bruxelles))
04/11/2020, 10:10
Paul Frederik Depta
(DESY)
04/11/2020, 10:30
Adil Jueid
(Shanghai JiaoTong University/Shanghai Key Laboratory for Partic)
04/11/2020, 10:50
Caterina Doglioni
(Lund University (SE))
04/11/2020, 11:10
Mr
Goran Jelic-Cizmek
(Universite de Geneve (CH))
Tutorials and demos
Tutorial
The 3-dimensional distribution of galaxies provides us with a powerful way of testing cosmological models. In order to extract information from this distribution, data has to be compressed using adequate estimators. One of the primary ones we use are the galaxy number counts, and its statistics: the 2-point correlation function, and its Fourier transform, the power spectrum. Past and current...
