985 citations · 11.4k across the 88 of their papers we have counts for
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Measuring the hydrostatic mass bias in galaxy clusters by combining Sunyaev-Zel'dovich and CMB lensing data
G. Hurier, R. E. Angulo
The cosmological parameters prefered by the cosmic microwave background (CMB) primary anisotropies predict many more galaxy clusters than those that have been detected via the ther…
The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the Intracluster Medium out to in Abell 2319
V. Ghirardini, S. Ettori, D. Eckert +5
We present the joint analysis of the X-ray and SZ signals in A2319, the galaxy cluster with the highest signal-to-noise ratio in Planck maps and that has been surveyed within our X…
Mapping the temperature of the intra-cluster medium with the tSZ effect
G. Hurier, C. Tchernin
The hot electrons in the intra-cluster medium produce a spectral distorsion of the cosmic microwave background (CMB) black body emission, the thermal Sunyaev-Zel'dovich effect (tSZ…
MILCANN : A neural network assessed tSZ map for galaxy cluster detection
G. Hurier, N. Aghanim, M. Douspis
We present the first combination of thermal Sunyaev-Zel'dovich (tSZ) map with a multi-frequency quality assessment of the sky pixels based on Artificial Neural Networks (ANN) aimin…
Constraining galaxy cluster velocity field with the tSZ-kSZ-kSZ bispectrum
G. Hurier
The Sunyaev-Zel'dovich (SZ) effects are produced by the interaction of cosmic microwave background (CMB) photons with the ionized and diffuse gas of electrons inside galaxy cluster…
Combined analysis of galaxy cluster number count, thermal Sunyaev-Zel'dovich power spectrum, and bispectrum
G. Hurier, F. Lacasa
The Sunyaev-Zel'dovich (SZ) effect is a powerful probe of the evolution of structures in the universe, and is thus highly sensitive to cosmological parameters and , thou…