Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Polarization Analysis
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June 2007 |
Pico: Parameters for the Impatient Cosmologist
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January 2007 |
Power spectra based Planck constraints on compensated isocurvature, and forecasts for LiteBIRD and CORE space missions
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April 2017 |
Planck 2015 results : X. Diffuse component separation: Foreground maps
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September 2016 |
Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models
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August 2000 |
Tilted physics: A cosmologically dipole-modulated sky
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July 2011 |
Planck 2015 results : XII. Full focal plane simulations
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September 2016 |
Likelihood Analysis of CMB Temperature and Polarization Power Spectra
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January 2008 |
Cosmological parameters from pre-planck cosmic microwave background measurements
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May 2013 |
HEALPix: A Framework for High‐Resolution Discretization and Fast Analysis of Data Distributed on the Sphere
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April 2005 |
Estimating the power spectrum of the cosmic microwave background
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February 1998 |
Planck 2013 results. XVI. Cosmological parameters
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October 2014 |
Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
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January 2012 |
The Atacama Cosmology Telescope: two-season ACTPol spectra and parameters
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June 2017 |
Planck 2018 results: I. Overview and the cosmological legacy of Planck
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September 2020 |
Myths and truths concerning estimation of power spectra: the case for a hybrid estimator
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April 2004 |
Planck 2018 results: IV. Diffuse component separation
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September 2020 |
Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
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April 2015 |
CMB polarization can constrain cosmology better than CMB temperature
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September 2014 |
Planck 2015 results : XI. CMB power spectra, likelihoods, and robustness of parameters
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September 2016 |
Planck pre-launch status: HFI beam expectations from the optical optimisation of the focal plane
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September 2010 |
Likelihood, Fisher information, and systematics of cosmic microwave background experiments
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January 2012 |
Planck 2015 results : XIII. Cosmological parameters
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September 2016 |
How to measure CMB polarization power spectra without losing information
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August 2001 |
Cosmological parameter constraints as derived from the Wilkinson Microwave Anisotropy Probe data via Gibbs sampling and the Blackwell-Rao estimator
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May 2005 |
Joint Bayesian Component Separation and CMB Power Spectrum Estimation
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March 2008 |
Planck 2018 results: VII. Isotropy and statistics of the CMB
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September 2020 |
Planck 2018 results: VIII. Gravitational lensing
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September 2020 |
Planck 2018 results: XII. Galactic astrophysics using polarized dust emission
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September 2020 |
Effect of aberration on partial-sky measurements of the cosmic microwave background temperature power spectrum
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January 2014 |
Planck 2018 results: X. Constraints on inflation
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September 2020 |
Modelling the correlation between the thermal Sunyaev Zel'dovich effect and the cosmic infrared background: tSZ–CIB correlation
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November 2012 |
SRoll2: an improved mapmaking approach to reduce large-scale systematic effects in the Planck High Frequency Instrument legacy maps
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September 2019 |
Fast estimation of polarization power spectra using correlation functions
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May 2004 |
Planck 2013 results. XV. CMB power spectra and likelihood
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October 2014 |
Inflationary features and shifts in cosmological parameters from Planck 2015 data
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October 2017 |
A Measurement of Secondary Cosmic Microwave Background Anisotropies with two Years of South pole Telescope Observations
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July 2012 |
A method for extracting maximum resolution power spectra from microwave sky maps
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May 1996 |
Cosmological parameters from CMB and other data: A Monte Carlo approach
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November 2002 |
Planck 2018 results: VI. Cosmological parameters
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September 2020 |
Planck pre-launch status: High Frequency Instrument polarization calibration
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September 2010 |
Planck 2013 results. VI. High Frequency Instrument data processing
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October 2014 |
Measurement of CIB power spectra over large sky areas from Planck HFI maps
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December 2016 |
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: FINAL MAPS AND RESULTS
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September 2013 |
Planck 2013 results. XI. All-sky model of thermal dust emission
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October 2014 |
TEASING: a fast and accurate approximation for the low multipole likelihood of the cosmic microwave background temperature
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November 2009 |
QuickPol: Fast calculation of effective beam matrices for CMB polarization
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January 2017 |
Planck intermediate results : XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth
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December 2016 |
Likelihood, Fisher information, and systematics of cosmic microwave background experiments
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June 2012 |
Measurements of the Temperature and E-mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
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January 2018 |
Planck intermediate results : LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
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November 2017 |
The Atacama Cosmology Telescope: likelihood for small-scale CMB data
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July 2013 |
Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
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October 2014 |
Do Baryons Trace Dark Matter in the Early Universe?
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December 2011 |
XSPECT, estimation of the angular power spectrum by computing cross-power spectra with analytical error bars
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April 2005 |
New estimates of the CMB angular power spectra from the WMAP 5 year low-resolution data
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November 2009 |
Planck 2018 results: II. Low Frequency Instrument data processing
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September 2020 |
Pico: Parameters for the Impatient Cosmologist
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January 2007 |
QUANTIFYING DISCORDANCE IN THE 2015 PLANCK CMB SPECTRUM
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February 2016 |
A CMB polarization primer
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October 1997 |
Three‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Implications for Cosmology
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June 2007 |
Planck intermediate results : XLI. A map of lensing-induced
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December 2016 |
Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation
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October 2014 |
Fast Spherical Harmonic Analysis: A Quick Algorithm for Generating and/or InvertingFull-Sky, High-Resolution Cosmic Microwave Background Anisotropy Maps
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October 1997 |
Compensated isocurvature perturbations and the cosmic microwave background
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December 2011 |
SRoll2: an improved mapmaking approach to reduce large-scale systematic effects in the Planck High Frequency Instrument legacy maps
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September 2019 |
WMAP 7 year constraints on CPT violation from large angle CMB anisotropies
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February 2012 |
Cosmic Microwave Background Likelihood Approximation by a Gaussianized Blackwell-Rao Estimator
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February 2009 |
Planck 2013 results. VII. HFI time response and beams
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October 2014 |
A simple empirically motivated template for the thermal Sunyaev-Zel’dovich effect
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May 2012 |
Planck 2015 results : VIII. High Frequency Instrument data processing: Calibration and maps
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September 2016 |
Residual noise covariance for Planck low-resolution data analysis
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November 2010 |
Planck 2015 results : XV. Gravitational lensing
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September 2016 |
Templates for the Sunyaev-Zel’Dovich Angular Power Spectrum
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January 2011 |
Likelihood analysis of CMB temperature and polarization power spectra
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May 2008 |
All-sky analysis of polarization in the microwave background
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February 1997 |
Hybrid estimation of cosmic microwave background polarization power spectra
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July 2006 |
MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets
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March 2002 |
Planck 2018 results: III. High Frequency Instrument data processing and frequency maps
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September 2020 |
Planck 2018 results: IX. Constraints on primordial non-Gaussianity
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September 2020 |
CMB Polarization can constrain cosmology better than CMB temperature
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text
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January 2014 |
Planck 2015 results : IX. Diffuse component separation: CMB maps
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September 2016 |
Planck 2018 results: XI. Polarized dust foregrounds
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September 2020 |
Power Spectra Based Planck Constraints on Compensated Isocurvature, and Forecasts for LiteBIRD and CORE Space Missions
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text
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January 2017 |
New estimates of the CMB angular power spectra from the WMAP 5 yrs low resolution data
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text
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January 2009 |
Reionization optical depth determination from Planck HFI data with ten percent accuracy
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March 2020 |
Statistics of cosmic microwave background polarization
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June 1997 |