Friday, January 6, 2012

1201.1282 (T. Biesiadzinski et al.)

Impact of Systematics on SZ-Optical Scaling Relations    [PDF]

T. Biesiadzinski, J. J. McMahon, C. J. Miller, B. Nord, L. Shaw
One of the central goals of multi-wavelength galaxy cluster cosmology is to unite all cluster observables to form a consistent understanding of cluster mass. Here, we study the impact of systematic effects from optical cluster catalogs on stacked SZ signals. We show that the optically predicted Y-decrement can vary by as much as 50% based on the current 2 sigma systematic uncertainties in the observed mass-richness relationship. Mis-centering and impurities will suppress the SZ signal compared to expectations for a clean and perfectly centered optical sample, but to a lesser degree. We show that the level of these variations and suppression is dependent on the amount of systematics in the optical cluster catalogs. We also study luminosity-dependent sub-sampling of the optical catalog, which creates Malmquist-like effects that biases upwards the observed Y-decrement of the stacked signal. We show that the current Planck measurements of the Y-decrement around SDSS optical clusters and their X-ray counterparts are consistent with expectations after accounting for the 1sigma (2sigma) optical systematic uncertainties using the Johnston (Rozo) mass-richness relation.
View original: http://arxiv.org/abs/1201.1282

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