Kevin M. Huffenberger

TL;DR: In this article, the authors present an analysis of Planck satellite data on the Coma Cluster observed via the Sunyaev-Zeldovich effect, and they find that the Arnaud et al. universal pressure profile does not fit Coma, and that their pressure profile for merging systems provides a good fit of the data only at r R_500 than the mean pressure profile predicted by the simulations.

TL;DR: In this article, the cross-correlation signal between galaxy weak lensing and CMB lensing was measured at a significance level of 3.1$\sigma and the amplitude of the best-fit model with respect to the bestfit 2018 Planck cosmology was 0.81\pm 0.25$, consistent with the previous results.

TL;DR: In this article, the cross-correlation signal between galaxy weak lensing and CMB lensing was measured at a significance level of 3.1$\sigma and the amplitude of the best-fit model with respect to the bestfit 2018 Planck cosmology was 0.81\pm 0.25$, consistent with the previous results.

TL;DR: In this paper, a multi-wavelength analysis of eleven Sunyaev Zel'dovich effect (SZE)-selected galaxy clusters (ten with new data) from the Atacama Cosmology Telescope (ACT) southern survey is presented.

TL;DR: In this paper, the authors describe the processing of the 334 billion raw data samples from the High Frequency Instrument (hereafter HFI) which they performed to produce six temperature maps from the first 295 days of Planck-HFI survey data.