J
Justin I. Read
Researcher at University of Surrey
Publications - 164
Citations - 15158
Justin I. Read is an academic researcher from University of Surrey. The author has contributed to research in topics: Galaxy & Dark matter. The author has an hindex of 56, co-authored 164 publications receiving 13448 citations. Previous affiliations of Justin I. Read include University of Leicester & University of Zurich.
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Journal ArticleDOI
SPHS: Smoothed Particle Hydrodynamics with a higher order dissipation switch
TL;DR: In this article, the spatial derivative of the velocity divergence is used as a higher order dissipation switch to detect flow convergence before it occurs, which is second order accurate and can be used to solve mixing and recovering numerical convergence with increasing resolution.
Journal ArticleDOI
The MAGellanic Inter-Cloud project (MAGIC) I: Evidence for intermediate-age stellar populations in between the Magellanic Clouds
Noelia E. D. Noël,Noelia E. D. Noël,Noelia E. D. Noël,Blair C. Conn,Ricardo Carrera,Ricardo Carrera,Justin I. Read,Justin I. Read,Hans-Walter Rix,Andrew E. Dolphin +9 more
TL;DR: The MAGellanic Inter-Cloud program (MAGIC) as discussed by the authors uses a synthetic color-magnitude diagram (CMD) technique to detect the presence of intermediate-age and old stars in the inter-cloud region.
Posted Content
The Magellanic Inter-Cloud Project (MAGIC) II: Slicing up the Bridge
Noelia E. D. Noël,Blair C. Conn,Justin I. Read,Ricardo Carrera,Andrew E. Dolphin,Hans-Walter Rix +5 more
TL;DR: In this paper, the MAGIC II project aimed at probing the stellar populations in ten large fields located perpendicular to the main ridge-line of HI in the Inter-Cloud region.
Journal ArticleDOI
Limits on the local dark matter density
TL;DR: In this article, the authors used moments of the Jeans equations combined with a Monte Carlo Markov Chain (MCMC) technique to marginalise over the unknown parameters of the vertical motion of stars in the solar neighborhood.
Proceedings ArticleDOI
Measuring the local dark matter density
TL;DR: In this article, the authors examined systematic problems in determining the local matter density from the vertical motion of stars, i.e., the "Oort limit", and determined the data quality required to detect local dark matter at its expected density.