Details

Autor(en) / Beteiligte

• MARRONE, Daniel P
• SMITH, Graham P
• HENNESSY, Ryan
• JOY, Marshall
• LAMB, James W
• LEITCH, Erik M
• MARTINO, Rossella
• MAZZOTTA, Pasquale
• MILLER, Amber
• MROCZKOWSKI, Tony
• MUCHOVEJ, Stephen
• PLAGGE, Thomas
• OKABE, Nobuhiro
• PRYKE, Clem
• SANDERSON, Alastair J. R
• TAKADA, Masahiro
• WOODY, David
• ZHANG, Yuying
• BONAMENTE, Massimiliano
• CARLSTROM, John E
• CULVERHOUSE, Thomas L
• GRALLA, Megan
• GREER, Christopher H
• HASLER, Nicole
• HAWKINS, David

Titel

LoCuSS: THE SUNYAEV―ZEL'DOVICH EFFECT AND WEAK-LENSING MASS SCALING RELATION

Ist Teil von

• The Astrophysical journal, 2012-08, Vol.754 (2), p.1-13

Ort / Verlag

Bristol: IOP

Erscheinungsjahr

2012

Quelle

EZB Free E-Journals

Beschreibungen/Notizen

• We present the first weak-lensing-based scaling relation between galaxy cluster mass, M sub(WL), and integrated Compton parameter Y sub(sph). Observations of 18 galaxy clusters at z [Asymptotically = to] 0.2 were obtained with the Subaru 8.2 m telescope and the Sunyaev-Zel'dovich Array. The M sub(WL)-Y sub(sph) scaling relations, measured at Delta = 500, 1000, and 2500 [rho] sub(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 sub(WL) at fixed Y sub(sph) of 20%, larger than both previous measurements of M sub(HSE)-Y sub(sph) scatter as well as the scatter in true mass at fixed Y sub(sph) found in simulations. Moreover, the scatter in our lensing-based scaling relations is morphology dependent, with 30%-40% larger M sub(WL) for undisturbed compared to disturbed clusters at the same Y sub(sph) at r sub(500). Further examination suggests that the segregation may be explained by the inability of our spherical lens models to faithfully describe the three-dimensional structure of the clusters, in particular, the structure along the line of sight. We find that the ellipticity of the brightest cluster galaxy, a proxy for halo orientation, correlates well with the offset in mass from the mean scaling relation, which supports this picture. This provides empirical evidence that line-of-sight projection effects are an important systematic uncertainty in lensing-based scaling relations.