Modified gravity and large scale flows, a review
Astrophysics and Space Science | SPRINGER | Published : 2017
Awarded by Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)
Participants in the recent Large Scale Flows conference would like to thank Roland Triay and ICISE in Vietnam. I acknowledge NED<SUP>8</SUP> and thank Lucas Macri and Pirin Erdogdu for making data available. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. Data used in this work was generated using Swinburne University's Theoretical Astrophysical Observatory (TAO). TAO is part of the Australian All-Sky Virtual Observatory (ASVO) and is freely accessible at https://tao.asvo.org.au. The Millennium Simulation was carried out by the Virgo Supercomputing Consortium at the Computing Centre of the Max Planck Society in Garching. It is publicly available at http://www.mpa-garching.mpg.de/Millennium/. The Semi-Analytic Galaxy Evolution ( SAGE) model used in this work is a publicly available codebase that runs on the dark matter halo trees of a cosmological N-body simulation. It is available for download at https://github.com/darrencroton/sage.