activity
20082025
most citedPlanck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

721 citations · 4.6k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.CO2025

ZTF SNe Ia DR2: Towards cosmology-grade ZTF supernova light curves using scene modeling photometry

L. Lacroix, N. Regnault, T. de Jaeger +36

The Zwicky Transient Facility (ZTF) is conducting a wide-field survey of the northern sky in three optical bands and the collaboration cosmology working group has released 3628 spe…

astro-ph.CO2024★ 45 cited

LISA Definition Study Report

Monica Colpi, Karsten Danzmann, Martin Hewitson +108

The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to detect and study gravitational waves from space. LISA will survey the sky for Gravitational Waves…

astro-ph.SR2023★ 15 cited

LISA Galactic binaries with astrometry from Gaia DR3

Thomas Kupfer, Valeriya Korol, Tyson B. Littenberg +11

Galactic compact binaries with orbital periods shorter than a few hours emit detectable gravitational waves at low frequencies. Their gravitational wave signals can be detected wit…

astro-ph.IM2022★ 8 cited

Adaptive Kernel Density Estimation proposal in gravitational wave data analysis

Mikel Falxa, Stanislav Babak, Maude Le Jeune

Markov Chain Monte Carlo approach is frequently used within Bayesian framework to sample the target posterior distribution. Its efficiency strongly depends on the proposal used to…

astro-ph.GA2020★ 8 cited

Planck intermediate results. LV. Reliability and thermal properties of high-frequency sources in the Second Planck Catalogue of Compact Sources

Planck Collaboration, Y. Akrami, M. Ashdown +117

We describe an extension of the most recent version of the Planck Catalogue of Compact Sources (PCCS2), produced using a new multi-band Bayesian Extraction and Estimation Package (…

astro-ph.GA2018★ 203 cited

Planck 2018 results. XI. Polarized dust foregrounds

Planck Collaboration, Y. Akrami, M. Ashdown +131

The study of polarized dust emission has become entwined with the analysis of the cosmic microwave background (CMB) polarization. We use new Planck maps to characterize Galactic du…

astro-ph.CO2017★ 10 cited

Planck intermediate results. LIII. Detection of velocity dispersion from the kinetic Sunyaev-Zeldovich effect

Planck Collaboration, N. Aghanim, Y. Akrami +141

Using the full-mission data, we present a detection of the temperature (and therefore velocity) dispersion due to the kinetic Sunyaev-Zeldovich (kSZ) effect from clu…

astro-ph.EP2016★ 35 cited

Planck intermediate results. LII. Planet flux densities

Planck Collaboration, Y. Akrami, M. Ashdown +147

Measurements of flux density are described for five planets, Mars, Jupiter, Saturn, Uranus, and Neptune, across the six Planck High Frequency Instrument frequency bands (100-857 GH…

astro-ph.CO2016★ 352 cited

CMB-S4 Science Book, First Edition

Kevork N. Abazajian, Peter Adshead, Zeeshan Ahmed +83

This book lays out the scientific goals to be addressed by the next-generation ground-based cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated teles…

astro-ph.IM2016★ 38 cited

POLARBEAR-2: an instrument for CMB polarization measurements

Y. Inoue, P. Ade, Y. Akiba +83

POLARBEAR-2 (PB-2) is a cosmic microwave background (CMB) polarization experiment that will be located in the Atacama highland in Chile at an altitude of 5200 m. Its science goals…

astro-ph.CO2016★ 398 cited

Planck intermediate results. XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth

Planck Collaboration, N. Aghanim, M. Ashdown +170

This paper describes the identification, modelling, and removal of previously unexplained systematic effects in the polarization data of the Planck High Frequency Instrument (HFI)…

astro-ph.CO2016★ 69 cited

Planck intermediate results. XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies

Planck Collaboration, N. Aghanim, M. Ashdown +157

Using the Planck 2015 data release (PR2) temperature maps, we separate Galactic thermal dust emission from cosmic infrared background (CIB) anisotropies. For this purpose, we imple…

astro-ph.CO2016★ 27 cited

Planck intermediate results. XLIX. Parity-violation constraints from polarization data

Planck Collaboration, N. Aghanim, M. Ashdown +148

Parity violating extensions of the standard electromagnetic theory cause in vacuo rotation of the plane of polarization of propagating photons. This effect, also known as cosmic bi…

astro-ph.GA2016★ 25 cited

Planck intermediate results. XLIV. The structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap

Planck Collaboration, N. Aghanim, M. I. R. Alves +165

We study the statistical properties of interstellar dust polarization at high Galactic latitude, using the Stokes parameter Planck maps at 353 GHz. Our aim is to advance the unders…

astro-ph.IM2015★ 163 cited

The POLARBEAR-2 and the Simons Array Experiment

A. Suzuki, P. Ade, Y. Akiba +86

We present an overview of the design and status of the \Pb-2 and the Simons Array experiments. \Pb-2 is a Cosmic Microwave Background polarimetry experiment which aims to character…

astro-ph.CO2015★ 721 cited

Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Planck Collaboration, N. Aghanim, M. Arnaud +221

This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlations of CMB data, using the hybrid approach employed previously: pixel-based at $\e…

astro-ph.CO2015★ 281 cited

Planck 2015 results. X. Diffuse component separation: Foreground maps

Planck Collaboration, R. Adam, P. A. R. Ade +236

Planck has mapped the microwave sky in nine frequency bands between 30 and 857 GHz in temperature and seven bands between 30 and 353 GHz in polarization. In this paper we consider…

astro-ph.CO2015★ 263 cited

Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps

Planck Collaboration, R. Adam, P. A. R. Ade +223

This paper describes the processing applied to the Planck High Frequency Instrument (HFI) cleaned, time-ordered information to produce photometrically calibrated maps in temperatur…

astro-ph.IM2015★ 74 cited

Planck 2015 results. VII. HFI TOI and beam processing

Planck Collaboration, R. Adam, P. A. R. Ade +225

The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polari…

astro-ph.IM2014★ 8 cited

Development and characterization of the readout system for POLARBEAR-2

D. Barron, P. A. R. Ade, Y. Akiba +69

POLARBEAR-2 is a next-generation receiver for precision measurements of the polarization of the cosmic microwave background (Cosmic Microwave Background (CMB)). Scheduled to deploy…

astro-ph.CO2013★ 183 cited

Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum with the POLARBEAR experiment

POLARBEAR Collaboration, P. A. R. Ade, Y. Akiba +70

Gravitational lensing due to the large-scale distribution of matter in the cosmos distorts the primordial Cosmic Microwave Background (CMB) and thereby induces new, small-scale …

astro-ph.CO2013★ 94 cited

Evidence for Gravitational Lensing of the Cosmic Microwave Background Polarization from Cross-correlation with the Cosmic Infrared Background

POLARBEAR Collaboration, P. A. R. Ade, Y. Akiba +73

We reconstruct the gravitational lensing convergence signal from Cosmic Microwave Background (CMB) polarization data taken by the POLARBEAR experiment and cross-correlate it with C…

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★ 143 cited

Planck 2013 results. VIII. HFI photometric calibration and mapmaking

Planck Collaboration, P. A. R. Ade, N. Aghanim +223

This paper describes the processing applied to the HFI cleaned time-ordered data to produce photometrically calibrated maps. HFI observes the sky over a broad range of frequencies,…