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19982024
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 31.5k across the 180 of their papers we have counts for

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37 papers · 1 filter

astro-ph.GA2020★ 4 cited

A complete search for redshift z>6.5 quasars in the VIKING survey

R. Barnett, S. J. Warren, N. J. G. Cross +4

We present the results of a new, deeper, and complete search for high-redshift quasars over 977deg of the VISTA Kilo-Degree Infrared Galaxy (VIKING) survey. This ex…

astro-ph.GA2020★ 9 cited

Galaxy mass profiles from strong lensing III: The two-dimensional broken power-law model

Conor M. O'Riordan, Stephen J. Warren, Daniel J. Mortlock

When modelling strong gravitational lenses, i.e., where there are multiple images of the same source, the most widely used parameterisation for the mass profile in the lens galaxy…

astro-ph.GA2020★ 14 cited

Galaxy mass profiles from strong lensing II: The elliptical power-law model

Conor M. O'Riordan, Stephen J. Warren, Daniel J. Mortlock

We present a systematic analysis of the constraints on the mass profile slope obtainable when fitting a singular power-law ellipsoid model to a typical strong lensing obs…

astro-ph.GA2019★ 82 cited

Euclid preparation: V. Predicted yield of redshift 7<z<9 quasars from the wide survey

Euclid Collaboration, R. Barnett, S. J. Warren +126

We provide predictions of the yield of quasars from the Euclid wide survey, updating the calculation presented in the Euclid Red Book in several ways. We account for revisi…

astro-ph.GA2019★ 15 cited

Galaxy mass profiles from strong lensing I: The circular power-law model

Conor M. O'Riordan, Stephen J. Warren, Daniel J. Mortlock

In this series of papers we develop a formalism for constraining mass profiles in strong gravitational lenses with extended images, using fluxes in addition to positional informati…

astro-ph.GA2019★ 6 cited

Cosmic Dawn and Reionization: Astrophysics in the Final Frontier

Asantha Cooray, James Aguirre, Yacine Ali-Haimoud +71

The cosmic dawn and epoch of reionization mark the time period in the universe when stars, galaxies, and blackhole seeds first formed and the intergalactic medium changed from neut…

astro-ph.GA2017★ 49 cited

A deep search for metals near redshift 7: the line-of-sight towards ULAS J1120+0641

Sarah E. I. Bosman, George D. Becker, Martin G. Haehnelt +5

We present a search for metal absorption line systems at the highest redshifts to date using a deep (30h) VLT/X-Shooter spectrum of the z = 7.084 quasi-stellar object (QSO) ULAS J1…

astro-ph.GA2017★ 115 cited

The compact, ~1 kpc host galaxy of a quasar at z=7.1

Bram Venemans, Fabian Walter, Roberto Decarli +6

We present ALMA observations of the [CII] fine structure line and the underlying far-infrared (FIR) dust continuum emission in J1120+0641, the most distant quasar currently known (…

astro-ph.GA2015★ 26 cited

Planck intermediate results. XXXIX. The Planck list of high-redshift source candidates

Planck Collaboration, P. A. R. Ade, N. Aghanim +186

The Planck mission, thanks to its large frequency range and all-sky coverage, has a unique potential for systematically detecting the brightest, and rarest, submillimetre sources o…

astro-ph.GA2015★ 103 cited

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.GA2015★ 27 cited

Planck intermediate results. XXXVIII. E- and B-modes of dust polarization from the magnetized filamentary structure of the interstellar medium

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

The quest for a B-mode imprint from primordial gravity waves on the polarization of the cosmic microwave background (CMB) requires the characterization of foreground polarization f…

astro-ph.GA2015★ 46 cited

Planck intermediate results. XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE

Planck Collaboration, N. Aghanim, B. Altieri +183

[Abridged] We use the Planck all-sky submm and mm maps to search for rare sources distinguished by extreme brightness, a few hundreds of mJy, and their potential for being situated…

astro-ph.GA2015★ 101 cited

Planck 2015 results. XXVIII. The Planck Catalogue of Galactic Cold Clumps

Planck Collaboration, P. A. R. Ade, N. Aghanim +220

We present the Planck Catalogue of Galactic Cold Clumps (PGCC), an all-sky catalogue of Galactic cold clump candidates detected by Planck. This catalogue is the full version of the…

astro-ph.GA2015★ 422 cited

Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Planck Collaboration, P. A. R. Ade, N. Aghanim +195

Within ten nearby (d < 450 pc) Gould Belt molecular clouds we evaluate statistically the relative orientation between the magnetic field projected on the plane of sky, inferred fro…

astro-ph.GA2015★ 38 cited

Planck intermediate results. XXXIV. The magnetic field structure in the Rosette Nebula

Planck Collaboration, N. Aghanim, M. I. R. Alves +197

Planck has mapped the polarized dust emission over the whole sky, making it possible to trace the Galactic magnetic field structure that pervades the interstellar medium (ISM). We…

astro-ph.GA2014★ 69 cited

Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust

Planck Collaboration, R. Adam, P. A. R. Ade +199

The role of the magnetic field in the formation of the filamentary structures observed in the interstellar medium (ISM) is a debated topic. The Planck all-sky maps of linearly pola…

astro-ph.GA2014★ 30 cited

Planck intermediate results. XXXI. Microwave survey of Galactic supernova remnants

Planck Collaboration, M. Arnaud, M. Ashdown +160

The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants. Of these, 16 were detected in at least two Planck fre…

astro-ph.GA2014★ 46 cited

Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck

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

The Andromeda Galaxy (M31) is one of a few galaxies that has sufficient angular size on the sky to be resolved by the Planck satellite. Planck has detected M31 in all of its freque…

astro-ph.GA2014★ 51 cited

No excess of bright galaxies around the redshift 7.1 quasar ULAS J1120+0641

Chris Simpson, Daniel Mortlock, Stephen Warren +5

We present optical and near-infrared imaging of the field of the z=7.0842 quasar ULAS J112001.48+064124.3 taken with the Hubble Space Telescope. We use these data to search for gal…

astro-ph.GA2014★ 26 cited

Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data

Planck Collaboration, P. A. R. Ade, N. Aghanim +189

Planck data when combined with ancillary data provide a unique opportunity to separate the diffuse emission components of the inner Galaxy. The purpose of the paper is to elucidate…

astro-ph.GA2014★ 190 cited

Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization

Planck Collaboration, P. A. R. Ade, M. I. R. Alves +177

Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We make use of the Planck 353 GHz I, Q, and U Stokes maps as du…

astro-ph.GA2014★ 101 cited

Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible

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

The Planck survey provides unprecedented full-sky coverage of the submillimetre polarized emission from Galactic dust, bringing new constraints on the properties of dust. The dust…

astro-ph.GA2014★ 170 cited

Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence

Planck Collaboration, P. A. R. Ade, N. Aghanim +186

Polarized emission observed by Planck HFI at 353 GHz towards a sample of nearby fields is presented, focusing on the statistics of polarization fractions and angles . The po…

astro-ph.GA2014★ 18 cited

Planck intermediate results. XVIII The millimetre and sub-millimetre emission from planetary nebulae

Planck Collaboration, M. Arnaud, F. Atrio-Barandela +158

Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurement…