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Patrick J. McDonald

Researcher at University of British Columbia

Publications -  121
Citations -  4231

Patrick J. McDonald is an academic researcher from University of British Columbia. The author has contributed to research in topics: Hydrocephalus & Medicine. The author has an hindex of 25, co-authored 108 publications receiving 3780 citations. Previous affiliations of Patrick J. McDonald include University of Toronto & University of Manitoba.

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Cosmological parameters from combining the Lyman-α forest with CMB, galaxy clustering and SN constraints

TL;DR: In this article, the Ly-? forest power spectrum (LYA) was combined with high resolution spectra with cosmic microwave background (CMB) including three-year WMAP, and supernovae (SN) and galaxy clustering constraints to derive new constraints on cosmological parameters.
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Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS

TL;DR: In this paper, the power spectrum and bispectrum up to 4th order in the initial density perturbations were modeled as a Taylor series in the local mass density, with the unknown coefficients in the series treated as free bias parameters.
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Can sterile neutrinos be the dark matter

TL;DR: The Ly-alpha forest power spectrum measured by the Sloan Digital Sky Survey and high-resolution spectroscopy observations are used in combination with cosmic microwave background and galaxy clustering constraints to place limits on a sterile neutrino as a dark matter candidate in the warm dark matter scenario.
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Baryon Acoustic Oscillation Intensity Mapping of Dark Energy

TL;DR: In this paper, the authors show how the study of acoustic oscillation in the 21 cm brightness can be accomplished by economical three-dimensional intensity mapping, which is the starting point for a new class of dark energy experiments dedicated to large angular scale mapping of the radio sky, shedding light on dark energy.
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How to evade the sample variance limit on measurements of redshift-space distortions

TL;DR: In this article, the authors used multiple tracers of large-scale density with different biases to measure the redshift-space distortion parameter β ≡ b −1f ≡ b−1d−ln D/d −ln a (where D is the growth factor and a the expansion factor).