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- W1977222018 abstract "Wilkinson microwave anisotropy probe (WMAP) has provided us with the highest resolution all-sky maps of the cosmic microwave background (CMB). As a result of thermal Sunyaev–Zel’dovich effect, clusters of galaxies are imprinted as tiny, poorly resolved dips on top of primary CMB anisotropies in these maps. Here, I describe different efforts to extract the physics of intracluster medium (ICM) from the sea of primary CMB, through combining WMAP with low-redshift galaxy or X-ray cluster surveys. This finally culminates at a mean (universal) ICM pressure profile, which is for the first time directly constrained from WMAP 3 year maps, and leads to interesting constraints on the ICM baryonic budget." @default.
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- W1977222018 date "2006-12-01" @default.
- W1977222018 modified "2023-09-24" @default.
- W1977222018 title "Intracluster medium through three years of WMAP" @default.
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- W1977222018 doi "https://doi.org/10.1016/j.newar.2006.09.022" @default.
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