Statistical properties of SZ and X-ray cluster detections
F. Pace, M. Maturi, M. Bartelmann, N. Cappelluti, K. Dolag, M., Meneghetti, L. Moscardini

TL;DR
This study calibrates galaxy cluster detection methods using simulated SZ and X-ray maps, demonstrating improved detection statistics with multi-band filtering and comparing detection thresholds, completeness, and contamination levels.
Contribution
It provides a detailed comparison of SZ and X-ray cluster detection properties, including calibration of detection thresholds, completeness, and contamination, using realistic simulations.
Findings
Multi-band filtering enhances SZ detection statistics.
ACT-like observations detect clusters with M>6-9e13 M_sun/h, 50% completeness at ~1e14 M_sun/h.
X-ray detection thresholds increase steeply with redshift, unlike SZ detections.
Abstract
Aims. We calibrate the number density, completeness, reliability and the lower mass limit of galaxy-cluster detections through their thermal SZ signal, and compare them to X-ray cluster detections. Methods. We simulate maps of the thermal SZ effect and the X-ray emission from light cones constructed in a large, hydrodynamical, cosmological simulation volume, including realistic noise contributions. The maps are convolved with linear, optimised, single- and multi-band filters to identify local peaks and their signal-to-noise ratios. The resulting peak catalogues are then compared to the halo population in the simulation volume to identify true and spurious detections. Results. Multi-band filtering improves the statistics of SZ cluster detections considerably compared to single-band filtering. Observations with the characteristics of ACT detect clusters with masses M>6-9e13 M_o/h,…
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