activity
20152025
most citedA wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecast

76 citations · 280 across the 30 of their papers we have counts for

collaborators

31 papers

astro-ph.CO2025

The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture Telescopes

The Simons Observatory Collaboration, I. Abril-Cabezas, S. Adachi +479

We present updated forecasts for the scientific performance of the degree-scale (0.5 deg FWHM at 93 GHz), deep-field survey to be conducted by the Simons Observatory (SO). By 2027,…

astro-ph.GA2023★ 1 cited

Constraining Millimeter Dust Emission in Nearby Galaxies with NIKA2: the case of NGC2146 and NGC2976

G. Ejlali, R. Adam, P. Ade +57

This study presents the first millimeter continuum mapping observations of two nearby galaxies, the starburst spiral galaxy NGC2146 and the dwarf galaxy NGC2976, at 1.15 mm and 2 m…

astro-ph.CO2023★ 1 cited

Systematic effects on the upcoming NIKA2 LPSZ scaling relation

A. Moyer-Anin, R. Adam, P. Ade +49

In cluster cosmology, cluster masses are the main parameter of interest. They are needed to constrain cosmological parameters through the cluster number count. As the mass is not a…

astro-ph.GA2023★ 12 cited

The stratification of ISM properties in the edge-on galaxy NGC 891 revealed by NIKA2

S. Katsioli, E. M. Xilouris, C. Kramer +60

As the millimeter wavelength range remains a largely unexplored spectral region for galaxies, the IMEGIN large program aims to map the millimeter continuum emission of 22 nearby ga…

astro-ph.GA2023★ 18 cited

NIKA2 Cosmological Legacy Survey: Survey Description and Galaxy Number Counts

L. Bing, M. Béthermin, G. Lagache +48

Aims. Deep millimeter surveys are necessary to probe the dust-obscured galaxies at high redshift. We conducted a large observing program at 1.2 and 2 mm with the NIKA2 camera insta…

astro-ph.HE2023★ 9 cited

Simultaneous Millimeter-wave, Gamma-ray, and Optical Monitoring of the Blazar PKS 2326-502 During a Flaring State

J. C. Hood, A. Simpson, A. McDaniel +66

Including millimeter-wave (mm-wave) data in multi-wavelength studies of the variability of active galactic nuclei (AGN) can provide insights into AGN physics that are not easily ac…

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.GA2021

Galactic Star Formation with NIKA2 (GASTON): Evidence of mass accretion onto dense clumps

A. J. Rigby, R. Adam, P. Ade +49

High-mass stars () play a crucial role in the evolution of galaxies, and so it is imperative that we understand how they are formed. We have used the New…

astro-ph.IM2021★ 1 cited

In-flight gain monitoring of SPIDER's transition-edge sensor arrays

J. P. Filippini, A. E. Gambrel, A. S. Rahlin +67

Experiments deploying large arrays of transition-edge sensors (TESs) often require a robust method to monitor gain variations with minimal loss of observing time. We propose a sens…

astro-ph.IM2021

BICEP Array: 150 GHz detector module development

A. Schillaci, P. A. R. Ade, Z. Ahmed +81

The BICEP/Keck Collaboration is currently leading the quest to the highest sensitivity measurements of the polarized CMB anisotropies on degree scale with a series of cryogenic tel…

astro-ph.IM2021★ 4 cited

Probing the role of magnetic fields in star-forming filaments: NIKA2-Pol commissioning results toward OMC-1

H. Ajeddig, R. Adam, P. Ade +43

Dust polarization observations are a powerful, practical tool to probe the geometry (and to some extent, the strength) of magnetic fields in star-forming regions. In particular, Pl…

astro-ph.CO2021★ 2 cited

PSZ2G091:A massive double cluster at z=0.822 observed by the NIKA2 camera

E. Artis, R. Adam, P. Ade +48

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

astro-ph.GA2021★ 1 cited

Dust Emission in Galaxies at Millimeter Wavelengths: Cooling of star forming regions in NGC6946

G. Ejlali, R. Adam, P. Ade +54

Interstellar dust plays an important role in the formation of molecular gas and the heating and cooling of the interstellar medium. The spatial distribution of the mm-wavelength du…

astro-ph.GA2021★ 8 cited

Galactic star formation with NIKA2 (GASTON): Filament convergence and its link to star formation

N. Peretto, R. Adam, P. Ade +45

In the past decade filaments have been recognised as a major structural element of the interstellar medium, the densest of these filaments hosting the formation of most stars. In s…

astro-ph.CO2021★ 2 cited

Crab nebula at 260 GHz with the NIKA2 polarimeter. Implications for the polarization angle calibration of future CMB experiments

A. Ritacco, R. Adam, P. Ade +43

The quest for primordial gravitational waves enclosed in the Cosmic Microwave Background (CMB) polarization B-modes signal motivates the development of a new generation of high sen…

astro-ph.GA2021

Overdensity of SubMillimiter Galaxies in the GJ526 Field mapped with the NIKA2 Camera

J. -F. Lestrade, R. Adam, P. Ade +43

Using the NIKA2 dual band millimeter camera installed on the IRAM30m telescope, we have mapped a relatively large field (~70 arcmin^2) in the direction of the star GJ526 to investi…

astro-ph.GA2021★ 2 cited

Exploring the millimetre emission in nearby galaxies: analysis of the edge-on galaxy NGC 891

S. Katsioli, R. Adam, P. Ade +54

New observations of the edge-on galaxy NGC 891, at 1.15 and 2 mm obtained with the IRAM 30-m telescope and the NIKA2 camera, within the framework of the IMEGIN (Interpreting the Mi…

astro-ph.CO2021★ 7 cited

The NIKA2 Sunyaev-Zeldovich Large Program

L. Perotto, R. Adam, P. Ade +48

The NIKA2 Guaranteed-Time SZ Large Program (LPSZ) is dedicated to the high-angular resolution SZ mapping of a representative sample of 45 SZ-selected galaxy clusters drawn from the…

astro-ph.CO2021★ 2 cited

The LPSZ-CLASH galaxy cluster sample: combining lensing and hydrostatic mass estimates

M. Muñoz-Echeverría, R. Adam, P. Ade +48

Starting from the clusters included in the NIKA sample and in the NIKA2 Sunyaev-Zel'dovich Large Program (LPSZ) we have selected a sample of six common objects with the Cluster Len…

astro-ph.CO2021

Multi-probe analysis of the galaxy cluster CL J1226.9+3332: hydrostatic mass and hydrostatic-to-lensing bias

M. Muñoz-Echeverría, R. Adam, P. Ade +48

We present a multi-probe analysis of the well-known galaxy cluster CL J1226.9+3332 as a proof of concept for multi-wavelength studies within the framework of the NIKA2 Sunyaev-Zeld…

astro-ph.CO2021

Mapping the intracluster medium temperature in the era of NIKA2 and MUSTANG-2

F. Ruppin, R. Adam, P. Ade +50

We present preliminary results from an on-going program that aims at mapping the intracluster medium (ICM) temperature of high redshift galaxy clusters from the MaDCoWS sample usin…

astro-ph.GA2021

Searching for high-z DSFGs with NIKA2 and NOEMA

L. Bing, R. Adam, P. Ade +45

As the possible progenitors of passive galaxies at z=2-3, dusty star-forming galaxies (DSFGs) at z>4 provide a unique perspective to study the formation, assembly, and early quench…

astro-ph.IM2021★ 14 cited

CONCERTO at APEX: Installation and first phase of on-sky commissioning

A. Catalano, P. Ade, M. Aravena +40

CONCERTO (CarbON CII line in post-rEionisation and ReionisaTiOn) is a large field-of-view (FoV) spectro-imager that has been installed on the Cassegrain Cabin of Atacama Pathfinder…

astro-ph.IM2020★ 17 cited

QUBIC VIII: Optical design and performance

C. O'Sullivan, M. De Petris, G. Amico +126

The Q and U Bolometric Interferometer for Cosmology (QUBIC) is a ground-based experiment that aims to detect B-mode polarisation anisotropies in the CMB at angular scales around th…