output
19952026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing astro-ph.COShow all

133 papers · 1 filter

astro-ph.CO2025

Thermal Sunyaev-Zel'dovich effect at the core of CL J1226.9+3332 revealed by NOEMA

M. Muñoz-Echeverría, J. -F. Macías-Pérez, R. Neri +58

We present first detailed maps of the thermal Sunyaev-Zel'dovich (tSZ) effect on a cluster with the NOrthern Extended Millimeter Array (NOEMA). The high sensitivity of t…

astro-ph.CO2025★ 1 cited

Type Ia supernova growth-rate measurement with LSST simulations: intrinsic scatter systematics

Bastien Carreres, Rebecca C. Chen, Erik R. Peterson +9

Measurement of the growth rate of structures ($\fsig$) with Type Ia supernovae (\sns) will improve our understanding of the nature of dark energy and enable tests of general relati…

astro-ph.CO2025★ 2 cited

The uncommon intracluster medium features of the first massive clusters selected independently of their baryon content

S. Andreon, M. Radovich, A. Moretti +6

Our current knowledge of the thermodynamic properties of galaxy clusters comes primarily from detailed studies of clusters selected by their minority components: hot baryons. Most…

astro-ph.CO2024★ 2 cited

Exploiting the high-resolution NIKA2 data to study the intracluster medium and dynamical state of ACT-CL J0240.0+0116

A. Paliwal, M. De Petris, A. Ferragamo +54

Having a detailed knowledge of the intracluster medium (ICM) to infer the exact cluster physics such as the cluster dynamical state is crucial for cluster-based cosmological studie…

astro-ph.CO2024

Toward the first cosmological results of the NIKA2 Sunyaev-Zeldovich Large Program: The SZ-Mass scaling relation

A. Moyer-Anin, R. Adam, P. Ade +53

In Sunyaev-Zeldovich (SZ) cluster cosmology, two tools are needed to be able to exploit data from large scale surveys in the millimeter-wave domain. An accurate description of the…

astro-ph.CO2024★ 550 cited

Euclid. I. Overview of the Euclid mission

Euclid Collaboration, Y. Mellier, Abdurro'uf +1134

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Eucl…

astro-ph.CO2024★ 9 cited

Absolute reference for microwave polarization experiments -- The COSMOCal project and its proof of concept

A. Ritacco, L. Bizzarri, S. Savorgnano +25

The cosmic microwave background (CMB), a remnant of the Big Bang, provides unparalleled insights into the primordial universe, its energy content, and the origin of cosmic structur…

astro-ph.CO2023

NIKA2 observations of 3 low-mass galaxy clusters at : pressure profile and - relation

R. Adam, M. Ricci, D. Eckert +64

Three galaxy clusters selected from the XXL X-ray survey at high redshift and low mass ( and M) were observed with NIKA2 to imag…

astro-ph.CO2023★ 3 cited

The NIKA2 Sunyaev-Zeldovich Large Program: Sample and upcoming product public release

L. Perotto, R. Adam, P. Ade +52

The NIKA2 camera operating at the IRAM 30 m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zeldovich effect towards galaxy clusters at intermediate and…

astro-ph.CO2023★ 5 cited

The XXL Survey LI. Pressure profile and - scaling relation in three low-mass galaxy clusters at observed with NIKA2

R. Adam, M. Ricci, D. Eckert +64

The thermodynamical properties of the intracluster medium (ICM) are driven by scale-free gravitational collapse, but they also reflect the rich astrophysical processes at play in g…

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.CO2023★ 11 cited

CONCERTO: Extracting the power spectrum of the [C II ] emission line

M. Van Cuyck, N. Ponthieu, G. Lagache +21

CONCERTO is the first experiment to perform a [CII] line intensity mapping survey to target . Measuring the [CII] power spectrum allows us to study the role of dusty star-fo…

astro-ph.CO2022★ 1 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★ 16 cited

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

M. Muñoz-Echeverría, J. F. Macías-Pérez, G. W. Pratt +50

The precise estimation of the mass of galaxy clusters is a major issue for cosmology. Large galaxy cluster surveys rely on scaling laws that relate cluster observables to their mas…

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.CO2021★ 5 cited

The Three Hundred-NIKA2 Sunyaev-Zeldovich Large Program twin samples: Synthetic clusters to support real observations

A. Paliwal, E. Artis, W. Cui +12

The simulation database of THE THREE HUNDRED Project has been used to pick synthetic clusters of galaxies with properties close to the observational targets of the NIKA2 camera Sun…

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.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.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.CO2020★ 23 cited

Exploiting NIKA2/XMM-Newton imaging synergy for intermediate mass, high- galaxy clusters within the NIKA2 SZ Large Program

F. Kéruzoré, F. Mayet, G. W. Pratt +40

High-resolution mapping of the intra-cluster medium (ICM) up to high redshift and down to low masses is crucial to derive accurate mass estimates of the galaxy cluster and to under…

astro-ph.CO2020★ 11 cited

The XXL Survey XLIV. Sunyaev-Zel'dovich mapping of a low-mass cluster at z~1: a multi-wavelength approach

M. Ricci, R. Adam, D. Eckert +62

In this paper, we present resolved observations of the Sunyaev-Zel'dovich (SZ) effect, obtained with the NIKA2 camera, towards the cluster of galaxies XLSSC102, a relatively low-ma…