Publications by Lance Miller

Weak-lensing mass calibration of the Atacama Cosmology Telescope equatorial Sunyaev-Zeldovich cluster sample with the Canada-France-Hawaii telescope stripe 82 survey

Journal of Cosmology and Astroparticle Physics IOP Publishing 2016 (2016) 013-

N Battaglia, A Leauthaud, H Miyatake, M Hasselfield, MB Gralla, R Allison, JR Bond, E Calabrese, D Crichton, MJ Devlin, R Dünner, J Dunkley, T Erben, S Ferrara, M Halpern, M Hilton, JC Hill, AD Hincks, R Hložek, KM Huffenberger, JP Hughes, JP Kneib, A Kosowsky, M Makler, TA Marriage

Mass calibration uncertainty is the largest systematic effect for using clusters of galaxies to constrain cosmological parameters. We present weak lensing mass measurements from the Canada-France-Hawaii Telescope Stripe 82 Survey for galaxy clusters selected through their high signal-to-noise thermal Sunyaev-Zeldovich (tSZ) signal measured with the Atacama Cosmology Telescope (ACT). For a sample of 9 ACT clusters with a tSZ signal-to-noise greater than five the average weak lensing mass is (4.8±0.8) ×1014 Mo, consistent with the tSZ mass estimate of (4.70±1.0) ×1014 Mo which assumes a universal pressure profile for the cluster gas. Our results are consistent with previous weak-lensing measurements of tSZ-detected clusters from the Planck satellite. When comparing our results, we estimate the Eddington bias correction for the sample intersection of Planck and weak-lensing clusters which was previously excluded.

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