Cosmology with peculiar velocities: observational effects

P. Andersen, T. M. Davis, C. Howlett

Research output: Contribution to journalArticle

5 Citations (Scopus)
318 Downloads (Pure)

Abstract

n this paper we investigate how observational effects could possibly bias cosmological inferences from peculiar velocity measurements. Specifically, we look at how bulk flow measurements are compared with theoretical predictions. Usually bulk flow calculations try to approximate the flow that would occur in a sphere around the observer. Using the Horizon Run 2 simulation we show that the traditional methods for bulk flow estimation can overestimate the magnitude of the bulk flow for two reasons: when the survey geometry is not spherical (the data do not cover the whole sky), and when the observations undersample the velocity distributions. Our results may explain why several bulk flow measurements found bulk flow velocities that seem larger than those expected in standard Λ cold dark matter cosmologies. We recommend a different approach when comparing bulk flows to cosmological models, in which the theoretical prediction for each bulk flow measurement is calculated specifically for the geometry and sampling rate of that survey. This means that bulk flow values will not be comparable between surveys, but instead they are comparable with cosmological models, which is the more important measure.
Original languageEnglish
Pages (from-to)4083-4092
JournalMonthly Notices of the Royal Astronomical Society
Volume463
Issue number4
Early online date8 Sep 2016
DOIs
Publication statusPublished - 21 Dec 2016

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