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Measuring the galaxy-mass and galaxy-dust correlations through magnification and reddening
Journal article   Open access

Measuring the galaxy-mass and galaxy-dust correlations through magnification and reddening

Brice Ménard, Ryan Scranton, Masataka Fukugita and Gordon Richards
Monthly notices of the Royal Astronomical Society, v 405(2), pp 1025-1039
Sep 2011
url
https://doi.org/10.1111/j.1365-2966.2010.16486.xView
Published, Version of Record (VoR) Open

Abstract

gravitational lensing: weak dark matter dust, extinction
We present a simultaneous detection of gravitational magnification and dust reddening effects due to galactic haloes and large-scale structure. The measurement is based on correlating the brightness of ∼85 000 quasars at z > 1 with the position of 24 million galaxies at z∼ 0.3 derived from the Sloan Digital Sky Survey and is used to constrain the galaxy-mass and galaxy-dust correlation functions up to cosmological scales. The presence of dust is detected from 20 kpc to several Mpc, and we find its projected density to follow: Σdust∼r −0.8 p, a distribution similar to mass. On large scales, its wavelength dependence is described by RV ≃ 4.9 ± 3.2, consistent with interstellar dust. This, in turn, implies a cosmic dust density of Ωdust≃ 5 × 10−6, roughly half of which comes from dust in haloes of ∼L ★ galaxies. We estimate the resulting opacity of the Universe for various evolutionary models and find 〈AV 〉∼ 0.03 mag up to z= 0.5. We present magnification measurements, corrected for dust extinction, from which the galaxy-mass correlation function is inferred to give the mean surface mass density profile around galaxies Σ∼ 30(θ/1 arcmin)−0.8 h M⊙ pc−2 up to a radius of 10 Mpc, in agreement with gravitational shear estimates.

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Astronomy & Astrophysics
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