activity
20102021
most citedA Joint Analysis of BICEP2/Keck Array and Planck Data

985 citations · 11.4k across the 88 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

67 papers · 1 filter

astro-ph.CO2021★ 22 cited

PACT. II. Pressure profiles of galaxy clusters using Planck and ACT

E. Pointecouteau, I. Santiago-Bautista, M. Douspis +9

The pressure of hot gas in groups and clusters of galaxies is a key physical quantity, which is directly linked to the total mass of the halo and several other thermodynamical prop…

astro-ph.CO2019★ 2 cited

Evolution of the mass-richness relation for the redMaPPer catalog

G. Hurier

The accurate determination of the galaxy cluster mass-observable relations is one of the major challenge of modern astrophysics and cosmology. We present a new statistical methodol…

astro-ph.CO2019★ 3 cited

Cosmological constraints from the mass accretion rate I: galaxy cluster number count evolution

G. Hurier

Galaxy cluster number count has been proven to be a powerful cosmological probe. However, cosmological constraints established with galaxy cluster number count are highly dependent…

astro-ph.CO2019★ 36 cited

PACT I: Combining ACT and Planck data for optimal detection of tSZ signal

N. Aghanim, M. Douspis, G. Hurier +8

We present the optimal reconstruction of the thermal Sunyaev-Zel'dovich (tSZ) effect signal based on the combination of a heterogeneous dataset consisting of ACT and Planck data, w…

astro-ph.CO2018

Secondary CMB anisotropies from magnetized halos --I: Power spectra of the Faraday rotation angle and conversion rate

Nadège Lemarchand, Julien Grain, Guillaume Hurier +2

Magnetized plasmas within halos of galaxies leave their footprint on the polarized anisotropies of the cosmic microwave background. The two dominant effects for astrophysical halos…

astro-ph.CO2018★ 38 cited

Spitzer Planck Herschel Infrared Cluster (SPHerIC) survey: Candidate galaxy clusters at 1.3 < z < 3 selected by high star-formation rate

C. Martinache, A. Rettura, H. Dole +17

There is a lack of large samples of spectroscopically confirmed clusters and protoclusters at high redshifts, 1.5. Discovering and characterizing distant (proto-)clusters is im…