activity
20152021
most citedPlanck 2015 results. XVI. Isotropy and statistics of the CMB

428 citations · 1.9k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2021★ 1 cited

In-flight gain monitoring of SPIDER's transition-edge sensor arrays

J. P. Filippini, A. E. Gambrel, A. S. Rahlin +67

Experiments deploying large arrays of transition-edge sensors (TESs) often require a robust method to monitor gain variations with minimal loss of observing time. We propose a sens…

astro-ph.CO2021★ 7 cited

A Simulation-Based Method for Correcting Mode Coupling in CMB Angular Power Spectra

J. S. -Y. Leung, J. Hartley, J. M. Nagy +67

Modern CMB analysis pipelines regularly employ complex time-domain filters, beam models, masking, and other techniques during the production of sky maps and their corresponding ang…

astro-ph.CO2021★ 4 cited

The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps

A. E. Gambrel, A. S. Rahlin, X. Song +64

We present the XFaster analysis package. XFaster is a fast, iterative angular power spectrum estimator based on a diagonal approximation to the quadratic Fisher matrix estimator. X…

astro-ph.CO2018★ 217 cited

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.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★ 56 cited

SPIDER: CMB polarimetry from the edge of space

R. Gualtieri, J. P. Filippini, P. A. R. Ade +61

SPIDER is a balloon-borne instrument designed to map the polarization of the millimeter-wave sky at large angular scales. SPIDER targets the B-mode signature of primordial gravitat…

astro-ph.IM2017★ 11 cited

280 GHz Focal Plane Unit Design and Characterization for the SPIDER-2 Suborbital Polarimeter

A. S. Bergman, P. A. R. Ade, S. Akers +76

We describe the construction and characterization of the 280 GHz bolometric focal plane units (FPUs) to be deployed on the second flight of the balloon-borne SPIDER instrument. The…

astro-ph.CO2017★ 45 cited

A New Limit on CMB Circular Polarization from SPIDER

J. M. Nagy, P. A. R. Ade, M. Amiri +58

We present a new upper limit on CMB circular polarization from the 2015 flight of SPIDER, a balloon-borne telescope designed to search for -mode linear polarization from cosmic…

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.CO2015★ 79 cited

Planck 2015 results. XII. Full Focal Plane simulations

Planck Collaboration, P. A. R. Ade, N. Aghanim +228

We present the 8th Full Focal Plane simulation set (FFP8), deployed in support of the Planck 2015 results. FFP8 consists of 10 fiducial mission realizations reduced to 18144 maps,…

astro-ph.CO2015★ 428 cited

Planck 2015 results. XVI. Isotropy and statistics of the CMB

Planck Collaboration, P. A. R. Ade, N. Aghanim +242

We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly…

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.CO2015★ 276 cited

Planck 2015 results. IX. Diffuse component separation: CMB maps

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

We present foreground-reduced CMB maps derived from the full Planck data set in both temperature and polarization. Compared to the corresponding Planck 2013 temperature sky maps, t…

astro-ph.CO2015★ 10 cited

Planck 2015 results. XX. Constraints on inflation

Planck Collaboration, P. A. R. Ade, N. Aghanim +244

We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the…

astro-ph.CO2015★ 372 cited

Planck 2015 results. XIV. Dark energy and modified gravity

Planck Collaboration, P. A. R. Ade, N. Aghanim +232

We study the implications of Planck data for models of dark energy (DE) and modified gravity (MG), beyond the cosmological constant scenario. We start with cases where the DE only…

astro-ph.IM2015★ 62 cited

Planck 2015 results. II. Low Frequency Instrument data processing

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

We present an updated description of the Planck Low Frequency Instrument (LFI) data processing pipeline, associated with the 2015 data release. We point out the places where our re…