Matches in SemOpenAlex for { <https://semopenalex.org/work/W4309136945> ?p ?o ?g. }
- W4309136945 endingPage "A149" @default.
- W4309136945 startingPage "A149" @default.
- W4309136945 abstract "Galaxies, diffuse gas, and dark matter make up the cosmic web that defines the large-scale structure of the Universe. We constrained the joint distribution of these constituents by cross-correlating galaxy samples binned by stellar mass from the Sloan Digital Sky Survey CMASS catalog with maps of lensing convergence and the thermal Sunyaev-Zeldovich (tSZ) effect from the Planck mission. Fitting a halo-based model to our measured angular power spectra (galaxy-galaxy, galaxy-lensing convergence, and galaxy-tSZ) at a median redshift of $z=0.53$, we detected variation with stellar mass of the galaxy satellite fraction and galaxy spatial distribution within host halos. We find a tSZ-halo hydrostatic mass bias, $b_h$, such that $(1-b_h)=0.6pm0.05$, with a hint of a larger bias, $b_h$, at the high stellar mass end. The normalization of the galaxy-cosmic microwave background lensing convergence cross-power spectrum shows that galaxies trace the matter distribution without an indication of stochasticity ($A=0.98pm 0.09$). We forecast that next-generation cosmic microwave background experiments will improve the constraints on the hydrostatic bias by a factor of two and will be able to constrain the small-scale distribution of dark matter, hence informing the theory of feedback processes." @default.
- W4309136945 created "2022-11-23" @default.
- W4309136945 creator A5021919464 @default.
- W4309136945 creator A5062119913 @default.
- W4309136945 date "2023-07-01" @default.
- W4309136945 modified "2023-09-30" @default.
- W4309136945 title "Cosmic census: Relative distributions of dark matter, galaxies, and diffuse gas" @default.
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