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- W1998342793 abstract "SZ clusters surveys like Planck, the South Pole Telescope, and the Atacama Cosmology Telescope, will soon be publishing several hundred SZ-selected systems. The key ingredient required to transport the mass calibration from current X-ray selected cluster samples to these SZ systems is the Ysz--Yx scaling relation. We constrain the amplitude, slope, and scatter of the Ysz--Yx scaling relation using SZ data from Planck, and X-ray data from Chandra. We find a best fit amplitude of ln (D_A^2Ysz/CY_X) = -0.202 pm 0.024 at the pivot point CY_X=8times 10^{-5} Mpc^2. This corresponds to a Ysz/Yx-ratio of 0.82pm 0.024, in good agreement with X-ray expectations after including the effects of gas clumping. The slope of the relation is alpha=0.916pm 0.032, consistent with unity at approx 2.3sigma. We are unable to detect intrinsic scatter, and find no evidence that the scaling relation depends on cluster dynamical state." @default.
- W1998342793 created "2016-06-24" @default.
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- W1998342793 date "2012-11-05" @default.
- W1998342793 modified "2023-09-23" @default.
- W1998342793 title "THEYSZ-YXSCALING RELATION AS DETERMINED FROMPLANCKANDCHANDRA" @default.
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- W1998342793 doi "https://doi.org/10.1088/0004-637x/760/1/67" @default.
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