Fast and Accurate Mocks: Getting the Most from Large Scale Structure Surveys

APA

Alvarez, M. (2016). Fast and Accurate Mocks: Getting the Most from Large Scale Structure Surveys. Perimeter Institute for Theoretical Physics. https://pirsa.org/16010079

MLA

Alvarez, Marcelo. Fast and Accurate Mocks: Getting the Most from Large Scale Structure Surveys. Perimeter Institute for Theoretical Physics, Jan. 21, 2016, https://pirsa.org/16010079

BibTex

          @misc{ scivideos_PIRSA:16010079,
            doi = {10.48660/16010079},
            url = {https://pirsa.org/16010079},
            author = {Alvarez, Marcelo},
            keywords = {Strong Gravity},
            language = {en},
            title = {Fast and Accurate Mocks: Getting the Most from Large Scale Structure Surveys},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2016},
            month = {jan},
            note = {PIRSA:16010079 see, \url{https://scivideos.org/pirsa/16010079}}
          }
          

Marcelo Alvarez Canadian Institute for Theoretical Astrophysics (CITA)

Source Repository PIRSA
Collection

Abstract

Generation of accurate mock observations tailored specifically to upcoming surveys such as Advanced ACT, CHIME, and LSST is a key technical challenge in cosmology. Traditional approaches involving N-body simulation are fraught with difficulties due to increasingly large survey volumes and depths. Typically, statistical ensembles can only be realized for a few carefully-chosen parameters, limiting exploration to a significantly restricted cosmological model space. We have developed a new massively parallel algorithm to generate accurate halo masses and positions in a fraction (~1e-3 to 1e-2) of the time taken by N-body simulations. I will present a suite of simulated full sky cluster Sunyaev-Zel’dovich maps that have been produced with this approach, and describe the types of virtual large scale structure observations that are now within reach in the coming years.