activity
20122018
most citedPlanck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts

482 citations · 2k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.CO2018★ 20 cited

Dust in galaxy clusters: Modeling at millimeter wavelengths and impact on Planck cluster cosmology

J. -B. Melin, J. G. Bartlett, Z. -Y. Cai +4

We have examined dust emission in galaxy clusters at millimeter wavelengths using the Planck map to constrain the model based on Herschel observations that was u…

astro-ph.GA2017★ 13 cited

The ESO's VLT Type Ia supernova spectral set of the final two years of SNLS

C. Balland, F. Cellier-Holzem, C. Lidman +24

We aim to present 70 spectra of 68 new high-redshift type Ia supernovae (SNeIa) measured at ESO's VLT during the final two years of operation (2006-2008) of the Supernova Legacy Su…

astro-ph.CO2017★ 19 cited

Exploring cosmic origins with CORE: mitigation of systematic effects

P. Natoli, M. Ashdown, R. Banerji +123

We present an analysis of the main systematic effects that could impact the measurement of CMB polarization with the proposed CORE space mission. We employ timeline-to-map simulati…

astro-ph.IM2017★ 124 cited

Exploring Cosmic Origins with CORE: Survey requirements and mission design

J. Delabrouille, P. de Bernardis, F. R. Bouchet +200

Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this p…

astro-ph.GA2017★ 108 cited

Dependence of Type Ia supernova luminosities on their local environment

Matthieu Roman, Delphine Hardin, Marc Betoule +18

We present a fully consistent catalog of local and global properties of host galaxies of 882 Type Ia supernovæ (SNIa) that were selected based on their light-curve properties, span…

astro-ph.IM2017★ 43 cited

Exploring Cosmic Origins with CORE: The Instrument

P. de Bernardis, P. A. R. Ade, J. J. A. Baselmans +126

We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is…

astro-ph.CO2017★ 24 cited

Exploring cosmic origins with CORE: effects of observer peculiar motion

C. Burigana, C. S. Carvalho, T. Trombetti +116

We discuss the effects on the CMB, CIB, and thermal SZ effect due to the peculiar motion of an observer with respect to the CMB rest frame, which induces boosting effects. We inves…

astro-ph.CO2017★ 75 cited

Exploring Cosmic Origins with CORE: B-mode Component Separation

M. Remazeilles, A. J. Banday, C. Baccigalupi +113

We demonstrate that, for the baseline design of the CORE satellite mission, the polarized foregrounds can be controlled at the level required to allow the detection of the primordi…

astro-ph.CO2017★ 28 cited

Exploring Cosmic Origins with CORE: Cluster Science

J. -B. Melin, A. Bonaldi, M. Remazeilles +118

We examine the cosmological constraints that can be achieved with a galaxy cluster survey with the future CORE space mission. Using realistic simulations of the millimeter sky, pro…

astro-ph.GA2016★ 33 cited

Exploring Cosmic Origins with CORE: Extragalactic sources in Cosmic Microwave Background maps

G. De Zotti, J. Gonzalez-Nuevo, M. Lopez-Caniego +121

We discuss the potential of a next generation space-borne Cosmic Microwave Background (CMB) experiment for studies of extragalactic sources. Our analysis has particular bearing on…

astro-ph.CO2016★ 7 cited

Galaxy clusters as probes for cosmology and dark matter

Elia S. Battistelli, Carlo Burigana, Paolo de Bernardis +8

In recent years, significant progress has been made in building new galaxy clusters samples, at low and high redshifts, from wide-area surveys, particularly exploiting the Sunyaev-…

astro-ph.CO2015★ 482 cited

Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts

Planck Collaboration, P. A. R. Ade, N. Aghanim +233

We present cluster counts and corresponding cosmological constraints from the Planck full mission data set. Our catalogue consists of 439 clusters detected via their Sunyaev-Zeldov…

astro-ph.CO2014★ 57 cited

Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope

Planck Collaboration, P. A. R. Ade, N. Aghanim +194

We present the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with the Russian-Turkish 1.5-m telescope (RTT150), as a part of the opt…

astro-ph.CO2013★ 218 cited

PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White Paper

PRISM Collaboration, Philippe André, Carlo Baccigalupi +140

PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Visio…

astro-ph.CO2013★ 293 cited

Planck 2013 results. XII. Component separation

Planck Collaboration, P. A. R. Ade, N. Aghanim +252

Planck has produced detailed all-sky observations over nine frequency bands between 30 and 857 GHz. These observations allow robust reconstruction of the primordial cosmic microwav…

astro-ph.CO2013★ 61 cited

Planck intermediate results. XIII. Constraints on peculiar velocities

Planck Collaboration, P. A. R. Ade, N. Aghanim +182

Using \Planck\ data combined with the Meta Catalogue of X-ray detected Clusters of galaxies (MCXC), we address the study of peculiar motions by searching for evidence of the kineti…

astro-ph.CO2012★ 52 cited

Planck intermediate results. VIII. Filaments between interacting clusters

Planck Collaboration, P. A. R. Ade, N. Aghanim +208

About half of the baryons of the Universe are expected to be in the form of filaments of hot and low density intergalactic medium. Most of these baryons remain undetected even by t…

astro-ph.CO2012★ 69 cited

Planck intermediate results. X. Physics of the hot gas in the Coma cluster

Planck Collaboration, P. A. R. Ade, N. Aghanim +207

We present an analysis of Planck satellite data on the Coma Cluster observed via the Sunyaev-Zeldovich effect. Planck is able, for the first time, to detect SZ emission up to r ~ 3…

astro-ph.CO2012★ 244 cited

The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

J. Delabrouille, M. Betoule, J. -B. Melin +39

We present the Planck Sky Model (PSM), a parametric model for the generation of all-sky, few arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, i…