activity
20162022
most citedThe NIKA2 large field-of-view millimeter continuum camera for the 30-m IRAM telescope

160 citations · 389 across the 21 of their papers we have counts for

collaborators

34 papers

astro-ph.CO202235 cited

A Deep Learning Approach to Infer Galaxy Cluster Masses from Planck Compton parameter maps

Daniel de Andres, Weiguang Cui, Florian Ruppin +8

Galaxy clusters are useful laboratories to investigate the evolution of the Universe, and accurately measuring their total masses allows us to constrain important cosmological para…

astro-ph.CO20221 cited

Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera

J. -F. Lestrade, F. -X. Desert, G. Lagache +44

Distinctive large-scale structures have been identified in the spatial distribution of optical galaxies up to redshift z ~ 1. In the more distant universe, the relationship between…

astro-ph.CO2022

Massive merging cluster PSZ2G091 as seen by the NIKA2 camera

E. Artis, R. Adam, P. Ade +49

PSZ2 G091.83+26.11 is a galaxy cluster with M500 = 7.43 x 10^14 Msun at z = 0.822 1. This object exhibits a complex morphology with a clear bimodality observed in X-rays. However,…

astro-ph.GA202213 cited

The Evolution of AGN Activity in Brightest Cluster Galaxies

T. Somboonpanyakul, M. McDonald, A. Noble +73

We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations on the full 2500 deg^2 South Pole Telescope (SPT)-SZ cluster sample. We describe a…

astro-ph.CO202118 cited

The History of Metal Enrichment Traced by X-ray Observations of High Redshift Galaxy Clusters

Anthony M. Flores, Adam B. Mantz, Steven W. Allen +7

We present the analysis of deep X-ray observations of 10 massive galaxy clusters at redshifts , with the primary goal of measuring the metallicity of the intraclus…

astro-ph.GA202124 cited

GASTON: Galactic Star Formation with NIKA2. Evidence for the mass growth of star-forming clumps

A. J. Rigby, N. Peretto, R. Adam +44

Determining the mechanism by which high-mass stars are formed is essential for our understanding of the energy budget and chemical evolution of galaxies. By using the New IRAM KIDs…