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

160 citations · 432 across the 22 of their papers we have counts for

collaborators

33 papers

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.CO20212 cited

Observations of compact sources in galaxy clusters using MUSTANG2

Simon R. Dicker, Elia S. Battistelli, Tanay Bhandarkar +26

Compact sources can cause scatter in the scaling relationships between the amplitude of the thermal Sunyaev-Zel'dovich Effect (tSZE) in galaxy clusters and cluster mass. Estimates…

astro-ph.GA202117 cited

Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT

John Orlowski-Scherer, Luca Di Mascolo, Tanay Bhandarkar +35

Galaxy clusters are an important tool for cosmology, and their detection and characterization are key goals for current and future surveys. Using data from the Wide-field Infrared…

astro-ph.CO202118 cited

Thermodynamic evolution of the galaxy cluster IDCS J1426.5+3508

S. Andreon, C. Romero, F. Castagna +8

We present resolved thermodynamic profiles out to 500 kpc, about , of the galaxy cluster IDCS J1426.5+3508 with 40 kpc resolution. Thanks to the combination of Su…

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…