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Sunyaev-Zel'dovich signal of the maxBCG SDSS galaxy clusters in WMAP
DOI: 10.1103/PhysRevD.85.023005 Bibcode: 2012PhRvD..85b3005D

Rozo, Eduardo; Hao, Jiangang; Dodelson, Scott +1 more

The Planck Collaboration measured the Sunyaev-Zel’dovich decrement of optically selected clusters from the Sloan Digital Sky Survey, finding that it falls significantly below expectations based on existing mass calibration of the maxBCG galaxy clusters. Resolving this tension requires either the data to go up, or the theoretical expectations to co…

2012 Physical Review D
Planck 13
Constraints on non-Gaussianity from Sunyaev-Zeldovich cluster surveys
DOI: 10.1103/PhysRevD.86.123520 Bibcode: 2012PhRvD..86l3520M

Mak, Daisy S. Y.; Pierpaoli, Elena

We perform a Fisher matrix analysis to forecast the capability of ongoing and future Sunyaev-Zeldovich cluster surveys in constraining the deviations from Gaussian distribution of primordial density perturbations. We use the constraining power of the cluster number counts and clustering properties to forecast limits on the fNL parameter…

2012 Physical Review D
Planck 8
Amplitudes of thermal and kinetic Sunyaev-Zel'dovich signals from small-scale CMB anisotropies
DOI: 10.1103/PhysRevD.85.043015 Bibcode: 2012PhRvD..85d3015A

Melchiorri, Alessandro; Cooray, Asantha; Pagano, Luca +4 more

While the arcminute-scale cosmic microwave background (CMB) anisotropies are due to secondary effects, point sources dominate the total anisotropy power spectrum. At high frequencies the point sources are primarily in the form of dusty, star-forming galaxies. Both Herschel and Planck have recently measured the anisotropy power spectrum of cosmic i…

2012 Physical Review D
Herschel Planck 2