activity
20012022
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 14.1k across the 77 of their papers we have counts for

collaborators

77 papers

astro-ph.IM2022★ 1 cited

Performance of the polarization leakage correction in the PILOT data

J-Ph. Bernard, A. Bernard, H. Roussel +33

The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon-borne experiment that aims to measure the polarized emission of the…

astro-ph.GA2021★ 22 cited

Probing the structure of a massive filament: ArTeMiS 350 and 450 micron mapping of the integral-shaped filament in Orion A

F. Schuller, Ph. André, Y. Shimajiri +18

(abridged) Within the Orion A molecular cloud, the integral-shaped filament (ISF) is a prominent, degree-long structure of dense gas and dust, with clear signs of recent and on-goi…

astro-ph.GA2021★ 24 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…

astro-ph.GA2020★ 33 cited

The role of Galactic HII regions in the formation of filaments. High-resolution submilimeter imaging of RCW 120 with ArTéMiS

A. Zavagno, Ph. André, F. Schuller +13

Massive stars and their associated ionized (HII) regions could play a key role in the formation and evolution of filaments that host star formation. However, the properties of fila…

astro-ph.CO2019

NIKA: a mm camera for Sunyaev-Zel'dovich science in clusters of galaxies

J. F. Macías-Pérez, R. Adam, P. Ade +42

Clusters of galaxies, the largest bound objects in the Universe, constitute a cosmological probe of choice, which is sensitive to both dark matter and dark energy. Within this fram…

astro-ph.CO2019★ 2 cited

Mapping the gas thermodynamic properties of the massive cluster merger MOO J11421527 at z = 1.2

F. Ruppin, R. Adam, P. Ade +51

We present the results of the analysis of the very massive cluster MOO J11421527 at a redshift based on high angular resolution NIKA2 Sunyaev-Zel'dovich (SZ) and $Chan…