papers

Publications (121)

astro-ph.CO2013

Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation

Planck Collaboration, P. A. R. Ade, N. Aghanim +238

We present new measurements of CIB anisotropies using Planck. Combining HFI data with IRAS, the angular auto- and cross frequency power spectrum is measured from 143 to 3000 GHz, a…

astro-ph.CO2016

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.CO2016

Planck intermediate results. L. Evidence for spatial variation of the polarized thermal dust spectral energy distribution and implications for CMB -mode analysis

Planck Collaboration, N. Aghanim, M. Ashdown +156

The characterization of the Galactic foregrounds has been shown to be the main obstacle in the challenging quest to detect primordial B-modes in the polarized microwave sky. We mak…

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.GA2012

Planck Intermediate Results. IX. Detection of the Galactic haze with Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +181

Using precise full-sky observations from Planck, and applying several methods of component separation, we identify and characterize the emission from the Galactic "haze" at microwa…

astro-ph.CO2014

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,…

astro-ph.HE2024

The MeerKAT Massive Distant Clusters Survey: A Radio Halo in a Massive Galaxy Cluster at z = 1.23

S. P. Sikhosana, M. Hilton, G. Bernardi +9

In the current paradigm, high redshift radio halos are expected to be scarce due to inverse Compton energy losses and redshift dimming, which cause them to be intrinsically faint.…

astro-ph.CO2011

Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance

A. Mennella, M. Bersanelli, R. C. Butler +158

The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photo…

astro-ph.CO2011

The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey

T. A. Marriage, V. Acquaviva, P. A. R. Ade +68

We report on twenty-three clusters detected blindly as Sunyaev-Zel'dovich (SZ) decrements in a 148 GHz, 455 square-degree map of the southern sky made with data from the Atacama Co…

astro-ph.CO2014

Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

Planck Collaboration, R. Adam, P. A. R. Ade +230

The polarized thermal emission from Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background (CMB) at frequencies above 1…

astro-ph.CO2013

Planck 2013 results. XIX. The integrated Sachs-Wolfe effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +245

Based on CMB maps from the 2013 Planck Mission data release, this paper presents the detection of the ISW effect, i.e., the correlation between the CMB and large-scale evolving gra…

astro-ph.CO2022

From BeyondPlanck to Cosmoglobe: Preliminary -band analysis

D. J. Watts, M. Galloway, H. T. Ihle +40

We present the first application of the Cosmoglobe analysis framework by analyzing 9-year time-ordered observations using similar machinery as BeyondPlanck utilizes…

astro-ph.CO2017

Detection of the pairwise kinematic Sunyaev-Zel'dovich effect with BOSS DR11 and the Atacama Cosmology Telescope

F. De Bernardis, S. Aiola, E. M. Vavagiakis +55

We present a new measurement of the kinematic Sunyaev-Zeldovich effect using data from the Atacama Cosmology Telescope (ACT) and the Baryon Oscillation Spectroscopic Survey (BOSS).…

astro-ph.CO2014

Planck 2013 results. XXI. All-sky Compton parameter power spectrum and high-order statistics

Planck Collaboration, P. A. R. Ade, N. Aghanim +235

We have constructed the first all-sky map of the thermal Sunyaev-Zeldovich (tSZ) effect by applying specifically tailored component separation algorithms to the 100 to 857 GHz freq…

astro-ph.GA2011

Planck early results. XV. Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources

Planck Collaboration, J. Aatrokoski, P. A. R. Ade +246

Spectral energy distributions (SEDs) and radio continuum spectra are presented for a northern sample of 104 extragalactic radio sources, based on the Planck Early Release Compact S…

astro-ph.CO2011

Planck early results XIV: ERCSC validation and extreme radio sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +206

Planck's all sky surveys at 30-857 GHz provide an unprecedented opportunity to follow the radio spectra of a large sample of extragalactic sources to frequencies 2-20 times higher…

astro-ph.GA2026

The MeerKAT Massive Distant Clusters Survey: a search for diffuse radio emission in 30 massive SZ-selected clusters at

Dakalo G. Phuravhathu, M. Hilton, S. P. Sikhosana +10

We present the results of a search for diffuse radio emission in a uniformly selected sample of 30 of the most massive Sunyaev-Zel'dovich selected galaxy clusters at , provi…

astro-ph.CO2026

The Atacama Cosmology Telescope: DR6 Sunyaev-Zel'dovich Selected Galaxy Clusters Catalog

HSC Collaboration, M. Aguena, S. Aiola +98

We present the results of a search for galaxy clusters in the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) microwave sky maps covering 16293 square degrees in three frequ…

astro-ph.GA2016

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.CO2019

Planck 2018 results. X. Constraints on inflation

Planck Collaboration, Y. Akrami, F. Arroja +173

We report on the implications for cosmic inflation of the 2018 Release of the Planck CMB anisotropy measurements. The results are fully consistent with the two previous Planck cosm…

astro-ph.EP2016

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.CO2020

Planck intermediate results. LVII. Joint Planck LFI and HFI data processing

Planck Collaboration, Y. Akrami, K. J. Andersen +136

We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High…

astro-ph.CO2018

Planck 2018 results. III. High Frequency Instrument data processing and frequency maps

Planck Collaboration, N. Aghanim, Y. Akrami +152

This paper presents the High Frequency Instrument (HFI) data processing procedures for the Planck 2018 release. Major improvements in mapmaking have been achieved since the previou…

astro-ph.CO2016

Planck 2015 results. III. LFI systematic uncertainties

Planck Collaboration, P. A. R. Ade, J. Aumont +166

We present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results…

astro-ph.CO2009

The Sunyaev-Zel'dovich effect in WMAP data

J. M Diego, B. Partridge

Using WMAP 5 year data, we look for the average Sunyaev-Zel'dovich effect (SZE) signal from clusters of galaxies by stacking the regions around hundreds of known X-ray clusters. We…

astro-ph.GA2016

Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds

Planck Collaboration, P. A. R. Ade, N. Aghanim +238

(abridged) We discuss the Galactic foreground emission between 20 and 100GHz based on observations by Planck/WMAP. The Commander component-separation tool has been used to separate…

astro-ph.CO2012

Simultaneous Planck, Swift, and Fermi observations of X-ray and gamma-ray selected blazars

P. Giommi, G. Polenta, A. Lahteenmaki +92

We present simultaneous Planck, Swift, Fermi, and ground-based data for 105 blazars belonging to three samples with flux limits in the soft X-ray, hard X-ray, and gamma-ray bands.…

astro-ph.HE2025

A Search for Millimeter-Bright Blazars as Astrophysical Neutrino Sources

R. Abbasi, M. Ackermann, J. Adams +424

The powerful jets of blazars have been historically considered as likely sites of high-energy cosmic-ray acceleration. However, particulars of the launched jet and the locations of…

astro-ph.GA2020

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.IM2011

Planck Early Results: The Planck mission

Planck Collaboration, P. A. R. Ade, N. Aghanim +272

The European Space Agency's Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009. Its performance is well in li…

astro-ph.CO2022

BeyondPlanck I. Global Bayesian analysis of the Planck Low Frequency Instrument data

BeyondPlanck Collaboration, K. J. Andersen, R. Aurlien +42

We describe the BeyondPlanck project in terms of motivation, methodology and main products, and provide a guide to a set of companion papers that describe each result in fuller det…

astro-ph.CO2016

Absolute Calibration of the Radio Astronomy Flux Density Scale at 22 to 43 GHz Using Planck

B. Partridge, M. López-Caniego, R. A. Perley +5

The Planck mission detected thousands of extragalactic radio sources at frequencies from 28 to 857 GHz. Planck's calibration is absolute (in the sense that it is based on the satel…

astro-ph.CO2015

Planck 2015 results. VI. LFI mapmaking

Planck Collaboration, P. A. R. Ade, N. Aghanim +198

This paper describes the mapmaking procedure applied to Planck LFI (Low Frequency Instrument) data. The mapmaking step takes as input the calibrated timelines and pointing informat…

astro-ph.CO2020

The Atacama Cosmology Telescope: A Catalog of > 4000 Sunyaev-Zel'dovich Galaxy Clusters

M. Hilton, C. Sifón, S. Naess +146

We present a catalog of 4195 optically confirmed Sunyaev-Zel'dovich (SZ) selected galaxy clusters detected with signal-to-noise > 4 in 13,211 deg of sky surveyed by the Atacama…

astro-ph.GA2026

The MeerKAT Massive Distant Clusters Survey: detection of diffuse radio emission in galaxy clusters at

Dakalo G. Phuravhathu, M. Hilton, S. P. Sikhosana +11

Diffuse, low surface-brightness radio emission in merging galaxy clusters provides insights into cosmic structure formation, the growth of magnetic fields, and turbulence. This pap…

astro-ph.CO2014

Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +207

This paper presents the characterization of the in-flight beams, the beam window functions and the associated uncertainties for the Planck Low Frequency Instrument (LFI). Knowledge…

astro-ph.IM2015

Planck 2015 results. V. LFI calibration

Planck Collaboration, P. A. R. Ade, N. Aghanim +206

We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, cov…

astro-ph.CO2010

Planck pre-launch status: the Planck-LFI programme

N. Mandolesi, M. Bersanelli, R. C. Butler +140

This paper provides an overview of the Low Frequency Instrument (LFI) programme within the ESA Planck mission. The LFI instrument has been developed to produce high precision maps…

astro-ph.CO2018

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.CO2021

MERGHERS Pilot: MeerKAT discovery of diffuse emission in nine massive Sunyaev-Zel'dovich-selected galaxy clusters from ACT

K. Knowles, D. S. Pillay, S. Amodeo +26

The MeerKAT Exploration of Relics, Giant Halos, and Extragalactic Radio Sources (MERGHERS) survey is a planned project to study a large statistical sample of galaxy clusters with t…

astro-ph.CO2010

The Atacama Cosmology Telescope: A Measurement of the 600< ell <8000 Cosmic Microwave Background Power Spectrum at 148 GHz

J. W. Fowler, V. Acquaviva, P. A. R. Ade +69

We present a measurement of the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz. The measurement uses maps with 1.4' angular resolutio…

astro-ph.CO2022

BeyondPlanck XI. Bayesian CMB analysis with sample-based end-to-end error propagation

L. P. L. Colombo, J. R. Eskilt, S. Paradiso +36

We present posterior sample-based cosmic microwave background (CMB) constraints from Planck LFI and WMAP observations derived through global end-to-end Bayesian processing. We use…

astro-ph.CO2013

Planck intermediate results. VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHz

Planck Collaboration, P. A. R. Ade, N. Aghanim +188

(abridged for arXiv) We make use of the Planck all-sky survey to derive number counts and spectral indices of extragalactic sources -- infrared and radio sources -- from the Planck…

astro-ph.CO2015

Planck 2015 results. I. Overview of products and scientific results

Planck Collaboration, R. Adam, P. A. R. Ade +352

The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submilli…

astro-ph.CO2018

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.CO2020

Planck 2018 results. V. CMB power spectra and likelihoods

Planck Collaboration, N. Aghanim, Y. Akrami +165

This paper describes the 2018 Planck CMB likelihoods, following a hybrid approach similar to the 2015 one, with different approximations at low and high multipoles, and implementin…

astro-ph.CO2013

Long-term variability of extragalactic radio sources in the Planck Early Release Compact Source Catalogue

X. Chen, J. P. Rachen, M. Lopez-Caniego +5

Combining measurements taken using the Wilkinson Microwave Anisotropy Probe (WMAP) from 2001 to 2008 with measurements taken using Planck from 2009 to 2010, we investigate the long…

astro-ph.CO2011

Planck Early Results: Statistical properties of extragalactic radio sources in the Planck Early Release Compact Source Catalogue

Planck Collaboration, P. A. R. Ade, N. Aghanim +201

The data reported in Planck's Early Release Compact Source Catalogue (ERCSC) are exploited to measure the number counts (dN/dS) of extragalactic radio sources at 30, 44, 70, 100, 1…

astro-ph.CO2019

Planck 2018 results. IX. Constraints on primordial non-Gaussianity

Planck Collaboration, Y. Akrami, F. Arroja +157

We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare e…

astro-ph.GA2016

On the redshift distribution and physical properties of ACT-selected DSFGs

T. Su, T. A. Marriage, V. Asboth +25

We present multi-wavelength detections of nine candidate gravitationally-lensed dusty star-forming galaxies (DSFGs) selected at 218GHz (1.4mm) from the ACT equatorial survey. Among…

astro-ph.GA2019

The Atacama Cosmology Telescope: CO(J = 3 - 2) mapping and lens modeling of an ACT-selected dusty star-forming galaxy

J. Rivera, A. J. Baker, P. A. Gallardo +13

We report Northern Extended Millimeter Array (NOEMA) CO() observations of the dusty star-forming galaxy ACT-S\,J020941+001557 at , which was detected as an u…

astro-ph.CO2018

Planck intermediate results. LIV. The Planck Multi-frequency Catalogue of Non-thermal Sources

Planck Collaboration, Y. Akrami, F. Argüeso +138

This paper presents the Planck Multi-frequency Catalogue of Non-thermal (i.e. synchrotron-dominated) Sources (PCNT) observed between 30 and 857 GHz by the ESA Planck mission. This…

astro-ph.CO2016

Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +240

The Second Planck Catalogue of Compact Sources is a catalogue of sources detected in single-frequency maps from the full duration of the Planck mission and supersedes previous vers…

astro-ph.CO2022

BeyondPlanck VIII. Efficient Sidelobe Convolution and Correction through Spin Harmonics

M. Galloway, M. Reinecke, K. J. Andersen +35

We introduce a new formulation of the Conviqt convolution algorithm in terms of spin harmonics, and apply this to the problem of sidelobe correction for BeyondPlanck, the first end…

astro-ph.CO2022

BeyondPlanck VI. Noise characterization and modelling

H. T. Ihle, M. Bersanelli, C. Franceschet +38

We present a Bayesian method for estimating instrumental noise parameters and propagating noise uncertainties within the global BeyondPlanck Gibbs sampling framework, and apply thi…

astro-ph.HE2014

Radio-Gamma-ray connection and spectral evolution in 4C +49.22 (S4 1150+49): the Fermi, Swift and Planck view

S. Cutini, S. Ciprini, M. Orienti +23

The Large Area Telescope on board the Fermi Gamma-ray Space Telescope detected a strong gamma-ray flare on 2011 May 15 from a source identified as 4C 49.22, a flat spectrum radio q…

astro-ph.CO2010

The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra

J. Dunkley, R. Hlozek, J. Sievers +64

We present cosmological parameters derived from the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz and 218 GHz over 296 deg^2 with th…

astro-ph.CO2022

BeyondPlanck XVI. Limits on Large-Scale Polarized Anomalous Microwave Emission from Planck LFI and WMAP

D. Herman, B. Hensley, K. J. Andersen +35

We constrain the level of polarized anomalous microwave emission (AME) on large angular scales using LFI and polarization data within a Bayesian C…

astro-ph.CO2022

BeyondPlanck III. Commander3

M. Galloway, K. J. Andersen, R. Aurlien +35

We describe the computational infrastructure for end-to-end Bayesian CMB analysis implemented by the BeyondPlanck collaboration. This code is called commander3, and provides a stat…

astro-ph.CO2022

BeyondPlanck VII. Bayesian estimation of gain and absolute calibration for CMB experiments

E. Gjerløw, H. T. Ihle, S. Galeotta +35

We present a Bayesian calibration algorithm for CMB observations as implemented within the global end-to-end BeyondPlanck (BP) framework, and apply this to the Planck Low Frequency…

astro-ph.CO2013

The Atacama Cosmology Telescope: likelihood for small-scale CMB data

J. Dunkley, E. Calabrese, J. Sievers +32

The Atacama Cosmology Telescope has measured the angular power spectra of microwave fluctuations to arcminute scales at frequencies of 148 and 218 GHz, from three seasons of data.…

astro-ph.CO2019

Planck 2018 results. I. Overview and the cosmological legacy of Planck

Planck Collaboration, Y. Akrami, F. Arroja +188

The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave…

astro-ph.CO2019

Planck 2018 results. VIII. Gravitational lensing

Planck Collaboration, N. Aghanim, Y. Akrami +155

We present measurements of the cosmic microwave background (CMB) lensing potential using the final 2018 temperature and polarization data. We increase the signifi…

astro-ph.CO2022

BeyondPlanck XIII. Intensity foreground sampling, degeneracies, and priors

K. J. Andersen, D. Herman, R. Aurlien +41

We present the intensity foreground algorithms and model employed within the BeyondPlanck analysis framework. The BeyondPlanck analysis is aimed at integrating component separation…

astro-ph.CO2012

Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

Planck Collaboration, P. A. R. Ade, N. Aghanim +183

We examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal D_A^2 Y for a sample of 19 objects for which weak lensing (WL) mass measurements…

astro-ph.GA2011

Planck early results. XX. New light on anomalous microwave emission from spinning dust grains

Planck Collaboration, P. A. R. Ade, N. Aghanim +213

Anomalous microwave emission (AME) has been observed by numerous experiments in the frequency range ~10-60 GHz. Using Planck maps and multi-frequency ancillary data, we have constr…

astro-ph.IM2022

BeyondPlanck V. Minimal ADC Corrections for Planck LFI

D. Herman, R. A. Watson, K. J. Andersen +36

We describe the correction procedure for Analog-to-Digital Converter (ADC) differential non-linearities (DNL) adopted in the Bayesian end-to-end BeyondPlanck analysis framework. Th…

astro-ph.GA2018

Planck Observations of M33

C. T. Tibbs, F. P. Israel, R. J. Laureijs +4

We have performed a comprehensive investigation of the global integrated flux density of M33 from radio to ultraviolet wavelengths, finding that the data between 100 GHz and…

astro-ph.CO2016

Planck 2015 results. XIII. Cosmological parameters

Planck Collaboration, P. A. R. Ade, N. Aghanim +259

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary…

astro-ph.IM2010

ACTPol: A polarization-sensitive receiver for the Atacama Cosmology Telescope

M. D. Niemack, P. A. R. Ade, J. Aguirre +39

The six-meter Atacama Cosmology Telescope (ACT) in Chile was built to measure the cosmic microwave background (CMB) at arcminute angular scales. We are building a new polarization…

astro-ph.CO2013

Planck 2013 results. XXVIII. The Planck Catalogue of Compact Sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +240

The Planck Catalogue of Compact Sources (PCCS) is the catalogue of sources detected in the first 15 months of Planck operations, the "nominal" mission. It consists of nine single-f…

astro-ph.CO2022

BeyondPlanck X. Bandpass and beam leakage corrections

T. L. Svalheim, K. J. Andersen, R. Aurlien +36

We discuss the treatment of bandpass and beam leakage corrections in the Bayesian BeyondPlanck CMB analysis pipeline as applied to the Planck LFI measurements. As a preparatory ste…

astro-ph.CO2024

XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z=1.98 galaxy cluster

J. van Marrewijk, L. Di Mascolo, A. S. Gill +18

How protoclusters evolved from sparse galaxy overdensities to mature galaxy clusters is still not well understood. In this context, detecting and characterizing the hot ICM at high…

astro-ph.CO2014

Planck 2013 results. XVII. Gravitational lensing by large-scale structure

Planck Collaboration, P. A. R. Ade, N. Aghanim +235

On the arcminute angular scales probed by Planck, the CMB anisotropies are gently perturbed by gravitational lensing. Here we present a detailed study of this effect, detecting len…

astro-ph.CO2014

Planck 2013 results. III. LFI systematic uncertainties

Planck Collaboration, N. Aghanim, C. Armitage-Caplan +217

We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological…

astro-ph.CO2009

Wide-Field Imaging and Polarimetry for the Biggest and Brightest in the 20GHz Southern Sky

S. Burke-Spolaor, R. D. Ekers, M. Massardi +4

We present wide-field imaging and polarimetry at 20GHz of seven of the most extended, bright (Stot >= 0.50 Jy), high-frequency selected radio sources in the southern sky with decli…

astro-ph.CO2025

Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel'dovich observations with ACT and DESI photometric galaxies

B. Hadzhiyska, S. Ferraro, B. Ried Guachalla +70

Recent advances in cosmological observations have provided an unprecedented opportunity to investigate the distribution of baryons relative to the underlying matter. In this work,…

astro-ph.CO2022

BeyondPlanck XV. Polarized foreground emission between 30 and 70 GHz

T. L. Svalheim, K. J. Andersen, R. Aurlien +35

We constrain polarized foreground emission between 30 and 70 GHz with the Planck Low Frequency Instrument (LFI) and WMAP data within the global Bayesian BeyondPlanck framework. We…

astro-ph.CO2014

Planck 2013 results. XVI. Cosmological parameters

Planck Collaboration, P. A. R. Ade, N. Aghanim +261

We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. The Planck spectra at high multipoles are extremely well descr…

astro-ph.CO2020

Planck 2018 results. IV. Diffuse component separation

Planck Collaboration, Y. Akrami, M. Ashdown +150

We present full-sky maps of the cosmic microwave background (CMB) and polarized synchrotron and thermal dust emission, derived from the third set of Planck frequency maps. These pr…

astro-ph.CO2019

Astro2020 APC White Paper: The need for better tools to design future CMB experiments

G. Rocha, A. J. Banday, R. Belen Barreiro +27

This white paper addresses key challenges for the design of next-decade Cosmic Microwave Background (CMB) experiments, and for assessing their capability to extract cosmological in…

astro-ph.CO2011

Planck Early Results: The Planck View of Nearby Galaxies

Planck Collaboration, P. A. R. Ade, N. Aghanim +192

The all-sky coverage of the Planck Early Release Compact Source Catalogue (ERCSC) provides an unsurpassed survey of galaxies at submillimetre (submm) wavelengths, representing a ma…

astro-ph.CO2010

The Atacama Cosmology Telescope (ACT): Beam Profiles and First SZ Cluster Maps

A. D. Hincks, V. Acquaviva, P. Ade +69

The Atacama Cosmology Telescope (ACT) is currently observing the cosmic microwave background with arcminute resolution at 148 GHz, 218 GHz, and 277 GHz. In this paper, we present A…

astro-ph.CO2012

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…

astro-ph.CO2013

Planck 2013 results. XV. CMB power spectra and likelihood

Planck collaboration, P. A. R. Ade, N. Aghanim +257

We present the Planck likelihood, a complete statistical description of the two-point correlation function of the CMB temperature fluctuations. We use this likelihood to derive the…

astro-ph.CO2015

Planck 2015 results. XXIII. The thermal Sunyaev-Zeldovich effect--cosmic infrared background correlation

Planck Collaboration, P. A. R. Ade, N. Aghanim +199

We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrar…

astro-ph.CO2022

Polarization and variability of compact sources measured in Planck time-ordered data

G. Rocha, R. Keskitalo, B. Partridge +4

This paper introduces a new Planck Catalog of Polarized and Variable Compact Sources (PCCS-PV) comprising 153 sources, the majority of which are extragalactic. The data include bot…

astro-ph.IM2010

Planck pre-launch status: Design and description of the Low Frequency Instrument

M. Bersanelli, N. Mandolesi, R. C. Butler +109

In this paper we present the Low Frequency Instrument (LFI), designed and developed as part of the Planck space mission, the ESA program dedicated to precision imaging of the cosmi…

astro-ph.CO2020

Planck 2018 results. VII. Isotropy and Statistics of the CMB

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

Analysis of the Planck 2018 data set indicates that the statistical properties of the cosmic microwave background (CMB) temperature anisotropies are in excellent agreement with pre…

astro-ph.CO2021

The mass and galaxy distribution around SZ-selected clusters

T. Shin, B. Jain, S. Adhikari +136

We present measurements of the radial profiles of the mass and galaxy number density around Sunyaev-Zel'dovich-selected clusters using both weak lensing and galaxy counts. The clus…

astro-ph.CO2016

Planck intermediate results. XLVII. Planck constraints on reionization history

Planck Collaboration, R. Adam, N. Aghanim +163

We investigate constraints on cosmic reionization extracted from the Planck cosmic microwave background (CMB) data. We combine the Planck CMB anisotropy data in temperature with th…

astro-ph.CO2015

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.CO2014

Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts

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

We present constraints on cosmological parameters using number counts as a function of redshift for a sub-sample of 189 galaxy clusters from the Planck SZ (PSZ) catalogue. The PSZ…

astro-ph.CO2014

Planck 2013 results. I. Overview of products and scientific results

Planck Collaboration, P. A. R. Ade, N. Aghanim +398

The ESA's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sk…

astro-ph.CO2013

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.CO2015

A Joint Analysis of BICEP2/Keck Array and Planck Data

BICEP2/Keck, Planck Collaborations, : +276

We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg patch of sky centered on…

astro-ph.CO2018

Planck 2018 results. II. Low Frequency Instrument data processing

Planck Collaboration, Y. Akrami, F. Argüeso +148

We present a final description of the data-processing pipeline for the Planck, Low Frequency Instrument (LFI), implemented for the 2018 data release. Several improvements have been…

astro-ph.GA2016

Planck intermediate results. XLV. Radio spectra of northern extragalactic radio sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +202

Continuum spectra covering centimetre to submillimetre wavelengths are presented for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on f…

astro-ph.CO2021

Planck 2018 results. VI. Cosmological parameters

Planck Collaboration, N. Aghanim, Y. Akrami +179

We present cosmological parameter results from the final full-mission Planck measurements of the CMB anisotropies. We find good consistency with the standard spatially-flat 6-param…

astro-ph.CO2011

The Atacama Cosmology Telescope: Extragalactic Sources at 148 GHz in the 2008 Survey

T. A. Marriage, J. B. Juin, Y. -T. Lin +66

We report on extragalactic sources detected in a 455 square-degree map of the southern sky made with data at a frequency of 148 GHz from the Atacama Cosmology Telescope 2008 observ…