|
Evaluation of the performance of inexact GMRES
|
journal
|
February 2011 |
|
IV.—On Least Squares and Linear Combination of Observations
|
journal
|
January 1936 |
|
Detection of polarization in the cosmic microwave background using DASI
|
journal
|
December 2002 |
|
Planck 2013 results. XVI. Cosmological parameters
|
journal
|
October 2014 |
|
Statistical simulations of the dust foreground to cosmic microwave background polarization (Corrigendum)
|
journal
|
October 2018 |
|
Planck 2018 results: IV. Diffuse component separation
|
journal
|
September 2020 |
|
Planck 2018 results: VI. Cosmological parameters
|
journal
|
September 2020 |
|
Planck 2018 results: V. CMB power spectra and likelihoods
|
journal
|
September 2020 |
|
Planck intermediate results: LVII. Joint Planck LFI and HFI data processing
|
journal
|
November 2020 |
|
Structure in the COBE differential microwave radiometer first-year maps
|
journal
|
September 1992 |
|
Cosmic Microwave Background Component Separation by Parameter Estimation
|
journal
|
April 2006 |
|
BICEP2. II. Experiment And Three-Year Data Set
|
journal
|
August 2014 |
|
BICEP2/KECK ARRAY V: MEASUREMENTS OF B -MODE POLARIZATION AT DEGREE ANGULAR SCALES AND 150 GHz BY THE KECK ARRAY
|
journal
|
September 2015 |
|
A hybrid map-Cℓ component separation method for primordial CMB B-mode searches
|
journal
|
March 2023 |
|
Testing for spectral index variations in polarized CMB foregrounds
|
journal
|
October 2022 |
|
The Python Sky Model: software for simulating the Galactic microwave sky
|
journal
|
May 2017 |
|
A 3D model of polarized dust emission in the Milky Way
|
journal
|
January 2018 |
|
SPT-3G D1: Constraints on inflationary gravitational waves with two years of SPT-3G data
|
journal
|
December 2025 |
|
BICEP/ Keck XVIII: Measurement of BICEP3 polarization angles and consequences for constraining cosmic birefringence and inflation
|
journal
|
March 2025 |
|
Pseudo- C ℓ estimators which do not mix E and B modes
|
journal
|
October 2006 |
|
Constraints on Primordial Gravitational Waves Using P l a n c k , WMAP, and New BICEP2/ K e c k Observations through the 2015 Season
|
journal
|
November 2018 |
|
Nonparametric maximum likelihood component separation for CMB polarization data
|
journal
|
December 2023 |
|
Pixel domain implementation of the minimally informed CMB map foreground cleaning method
|
journal
|
November 2024 |
|
How to measure CMB power spectra without losing information
|
journal
|
May 1997 |
|
E/B decomposition of finite pixelized CMB maps
|
journal
|
January 2003 |
|
Likelihood analysis of CMB temperature and polarization power spectra
|
journal
|
May 2008 |
|
Polarized CMB power spectrum estimation using the pure pseudo-cross-spectrum approach
|
journal
|
June 2009 |
|
Forecasting performance of CMB experiments in the presence of complex foreground contaminations
|
journal
|
October 2016 |
|
Pure E and B polarization maps via Wiener filtering
|
journal
|
August 2017 |
|
Joint Analysis of BICEP2/ Keck Array and Planck Data
|
journal
|
March 2015 |
|
Dust-Polarization Maps for Local Interstellar Turbulence
|
journal
|
July 2018 |
|
Improved Constraints on Primordial Gravitational Waves using Planck , WMAP, and BICEP/ Keck Observations through the 2018 Observing Season
|
journal
|
October 2021 |
|
Maximum likelihood algorithm for parametric component separation in cosmic microwave background experiments
|
journal
|
January 2009 |
|
Templates for the Solution of Linear Systems: Building Blocks for Iterative Methods.
|
journal
|
July 1995 |
|
BICEP2/KECK ARRAY. VII. MATRIX BASED E/B SEPARATION APPLIED TO BICEP2 AND THE KECK ARRAY
|
journal
|
June 2016 |
|
CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
|
journal
|
February 2022 |
|
Bicep/Keck XV: The Bicep3 Cosmic Microwave Background Polarimeter and the First Three-year Data Set
|
journal
|
March 2022 |
|
BICEP/Keck. XVI. Characterizing Dust Polarization through Correlations with Neutral Hydrogen
|
journal
|
March 2023 |
|
Full-sky Models of Galactic Microwave Emission and Polarization at Subarcminute Scales for the Python Sky Model
|
journal
|
September 2025 |
|
CMB-S4: Foreground-cleaning Pipeline Comparison for Measuring Primordial Gravitational Waves
|
journal
|
October 2025 |