LoCuSS: The Sunyaev-Zel'dovich Effect and Weak Lensing Mass Scaling Relation
Daniel P. Marrone, Graham P. Smith, Nobuhiro Okabe, Massimiliano, Bonamente, John E. Carlstrom, Thomas L. Culverhouse, Megan Gralla,, Christopher H. Greer, Nicole Hasler, David Hawkins, Ryan Hennessy, Marshall, Joy, James W. Lamb, Erik M. Leitch, Rossella Martino

TL;DR
This study establishes a weak-lensing-based scaling relation between galaxy cluster mass and the Sunyaev-Zel'dovich effect, revealing a larger intrinsic scatter and morphology dependence, highlighting projection effects as a key systematic.
Contribution
First empirical weak-lensing mass-Y_sph scaling relation for galaxy clusters, demonstrating morphology dependence and the impact of projection effects on mass estimates.
Findings
Intrinsic scatter in M_wl at fixed Y_sph is about 20%.
Undisturbed clusters show 30-40% larger M_wl than disturbed ones at the same Y_sph.
Ellipticity of the brightest cluster galaxy correlates with mass offset, indicating projection effects.
Abstract
We present the first weak-lensing-based scaling relation between galaxy cluster mass, M_wl, and integrated Compton parameter Y_sph. Observations of 18 galaxy clusters at z~0.2 were obtained with the Subaru 8.2-m telescope and the Sunyaev-Zel'dovich Array. The M_wl-Y_sph scaling relations, measured at Delta=500, 1000, and 2500 rho_c, are consistent in slope and normalization with previous results derived under the assumption of hydrostatic equilibrium (HSE). We find an intrinsic scatter in M_wl at fixed Y_sph of 20%, larger than both previous measurements of M_HSE-Y_sph scatter as well as the scatter in true mass at fixed Y_sph found in simulations. Moreover, the scatter in our lensing-based scaling relations is morphology dependent, with 30-40% larger M_wl for undisturbed compared to disturbed clusters at the same Y_sph at r_500. Further examination suggests that the segregation may be…
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