MASTER of the CMB Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex CMB Data Sets

Abstract

We describe a fast and accurate method for estimation of the cosmic microwave background (CMB) anisotropy angular power spectrum --- Monte Carlo Apodised Spherical Transform EstimatoR. Originally devised for use in the interpretation of the Boomerang experimental data, MASTER is both a computationally efficient method suitable for use with the currently available CMB data sets (already large in size, despite covering small fractions of the sky, and affected by inhomogeneous and correlated noise), and a very promising application for the analysis of very large future CMB satellite mission products.

20 pages, 6 fig; submitted to ApJ; uses aastex.cls and psfig.sty (included)

References in corpus (3)

• A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data
• A Map-Making Algorithm for the Planck Surveyor
• MAPCUMBA : a fast iterative multi-grid map-making algorithm for CMB experiments

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• Separating weak lensing and intrinsic alignments using radio observations
• Optimal Estimation of the Binned Mask-Free Power Spectrum, Bispectrum, and Trispectrum on the Full Sky: Scalar Edition
• Constraints on non-resonant photon-axion conversion from the Planck satellite data
• Primordial Non-Gaussianity from a Joint Analysis of Cosmic Microwave Background Temperature and Polarization
• BeyondPlanck VI. Noise characterization and modelling
• Real-world CMB lensing quadratic estimator power spectrum response
• The Angular Power Spectrum of the First-Year WMAP Data Reanalysed
• Harmonic Inpainting of the Cosmic Microwave Background Sky: Formulation and Error Estimate
• A multi-level solver for Gaussian constrained CMB realizations
• POKER: Estimating the power spectrum of diffuse emission with complex masks and at high angular resolution
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• Catalog-based pseudo-$C_{\ell }$s
• Asymfast, a method for convolving maps with asymmetric main beams
• Correlated Component Analysis for diffuse component separation with error estimation on simulated Planck polarization data
• Isotropy statistics of CMB hot and cold spots
• WMAP 9-year CMB estimation using sparsity
• Optimization of foreground moment deprojection for semi-blind CMB polarization reconstruction
• A Generative Model of Galactic Dust Emission Using Variational Inference
• Bayesian angular power spectrum analysis of interferometric data
• Likelihood, Fisher information, and systematics of cosmic microwave background experiments
• Cross-Correlation of Near and Far-Infrared Background Anisotropies as Traced by Spitzer and Herschel
• Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear
• Integrated Sachs-Wolfe map recovery from NVSS and WMAP 7yr data
• Tomographic Constraints on Gravity from Angular Redshift Fluctuations in the Late Universe
• Angular power spectrum of the FastICA CMB component from BEAST data
• A novel approach to reconstructing signals of isotropy violation from a masked CMB sky
• Measurements of the Cross Spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz
• Galaxy Clustering in 3D and Modified Gravity Theories
• Consistency of cosmic microwave background temperature measurements in three frequency bands in the 2500-square-degree SPT-SZ survey
• Lensing covariance on cut sky and SPT-Planck lensing tensions
• Fast Parameter Estimation from the CMB Power Spectrum
• Disentangling Doppler modulation, aberration and the temperature dipole in the CMB
• The Impact of Anisotropic Redshift Distributions on Angular Clustering
• Constraining f(R) gravity with cross-correlation of galaxies and cosmic microwave background lensing
• Model independent approaches to reionization in the analysis of upcoming CMB data
• Data analysis methods for the cosmic microwave background
• Correlations Between the WMAP and MAXIMA Cosmic Microwave Background Anisotropy Maps
• Cosmo++: An Object-Oriented C++ Library for Cosmology
• Effects of Destriping Errors on CMB Polarisation Power Spectra and and Pixel Noise Covariances
• The star formation history in the last 10 billion years from CIB cross-correlations
• The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz
• The Morphology of the Thermal Sunyaev-Zel'dovich Sky
• CMB Polarization and Temperature Power Spectra Estimation using Linear Combination of WMAP 5-year Maps
• Inpainting CMB maps using Partial Convolutional Neural Networks
• ECLIPSE: a fast Quadratic Maximum Likelihood estimator for CMB intensity and polarization power spectra
• Hierarchical Bayesian CMB Component Separation with the No-U-Turn Sampler
• Angular power spectrum of CMB anisotropy from WMAP
• Removing beam asymmetry bias in precision CMB temperature and polarisation experiments
• Fast computation of angular power spectra and covariances of high-resolution cosmic microwave background maps using the Toeplitz approximation
• Optimal cosmic microwave background map-making in the presence of cross-correlated noise
• Lensing-induced morphology changes in CMB temperature maps in modified gravity theories
• Mitigating the impact of the CIB on galaxy cluster SZ detection with spectrally constrained matched filters
• LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
• Reassessment of the dipole in the distribution of quasars on the sky
• Measurements and implications of cosmic ray anisotropies from TeV to trans-EeV energies
• Subdegree Sunyaev-Zel'dovich Signal from Multifrequency BOOMERanG observations
• Exact joint likelihood of pseudo-$C_{\ell }$ estimates from correlated Gaussian cosmological fields
• Constraining low redshift [CII] Emission by Cross-Correlating FIRAS and BOSS Data
• ISW-LSS cross-correlation in coupled Dark Energy models with massive neutrinos
• Using CMB data to constrain non-isotropic Planck-scale modifications to Electrodynamics
• PRISM: Recovery of the primordial spectrum from Planck data
• Hemispherical asymmetry from an isotropy violating stochastic gravitational wave background
• Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlation with the cosmic microwave background
• Weak Lensing Skew-Spectrum
• Estimating the Integrated Bispectrum from Weak Lensing Maps
• Large angular scale fluctuations of near infrared extragalactic background light based on the IRTS observations
• Joint analyses of 2D CMB lensing and 3D galaxy clustering in the spherical Fourier-Bessel basis
• Linearized iterative least-squares (LIL): A parameter fitting algorithm for component separation in multifrequency CMB experiments such as Planck
• The Cosmic Microwave Background Radiation Power Spectrum as a Random Bit Generator for Symmetric and Asymmetric-Key Cryptography
• Fast calculation of the Fisher matrix for cosmic microwave background experiments
• Parametric tension between even and odd multipole data of WMAP power spectrum: unaccounted contamination or missing parameters?
• Constraining the Halo Mass of Damped Ly$\alpha$ Absorption Systems (DLAs) at $z=2-3.5$ using the Quasar-CMB Lensing Cross-correlation
• Impact of modelling foreground uncertainties on future CMB polarization satellite experiments
• Power spectrum sensitivity of raster-scanned CMB experiments in the presence of 1/f noise
• Constraints on primordial non-Gaussianity from the cross-correlation of DESI Luminous Red Galaxies and $Planck$ CMB lensing
• Noise power spectrum estimation and fast map making for CMB experiments
• Calibrating magnification bias for the $E_G$ statistic to test general relativity
• On the Coherence of WMAP and Planck Temperature Maps
• CMB power spectrum estimation with non-circular beam and incomplete sky coverage
• A cross-correlation analysis of CMB lensing and radio galaxy maps
• Environment from cross-correlations: connecting hot gas and the quenching of galaxies
• Marginal distributions for cosmic variance limited CMB polarization data
• Cross-correlation between $Planck$ CMB lensing potential and galaxy catalogues from HELP
• Leverage on small-scale primordial non-Gaussianity through cross-correlations between CMB $E$-mode and $\mu$-distortion anisotropies
• Constraining the physics of star formation from CIB-cosmic shear cross-correlations
• Needlet thresholding methods in component separation
• Constraints on dark matter and astrophysics from tomographic $\gamma$-ray cross-correlations
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• A measurement of the Integrated Sachs-Wolfe Effect with the Rapid ASKAP Continuum Survey
• Galaxy cluster SZ detection with unbiased noise estimation: an iterative approach
• Iterative map-making with two-level preconditioning for polarized Cosmic Microwave Background data sets
• Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
• Detection of Dipole Modulation in CMB Temperature Anisotropy Maps from WMAP and Planck using Artificial Intelligence
• Impact of Galactic dust non-Gaussianity on searches for B-modes from inflation
• Optimized Large-Scale CMB Likelihood And Quadratic Maximum Likelihood Power Spectrum Estimation
• Revisiting the large-scale CMB anomalies: The impact of the SZ signal from the Local Universe
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• A Generalized Doppler and Aberration Kernel for Frequency-Dependent Cosmological Observables
• Non-Circular beam correction to the CMB power spectrum
• Degree-scale anomalies in the CMB: localizing the first peak dip to a small patch of the north ecliptic sky
• Using peak distribution of the cosmic microwave background for MAP and Planck data analysis: formalism and simulations
• Direct measurement of the angular power spectrum of cosmic microwave background temperature anisotropies in the WMAP Data
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• Data driven foreground clustering approach to component separation in multifrequency CMB experiments: A new Planck CMB map
• Testing for foreground residuals in the Planck foreground cleaned maps: A new method for designing confidence masks
• Cross-correlation of POLARBEAR CMB Polarization Lensing with High-$z$ Sub-mm Herschel-ATLAS galaxies
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Weak Lensing Trispectrum and Kurt-Spectra
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Cosmological constraints from low redshift 21 cm intensity mapping with machine learning
• CMB lensing reconstruction with point source masks
• Euclid preparation. LIX. Angular power spectra from discrete observations
• The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra
• CMB Power Spectrum Estimation for the Planck Surveyor
• Consistency of CMB experiments beyond cosmic variance
• The BINGO project VIII: On the recoverability of the BAO signal on HI intensity mapping simulations
• Foreground Maps in WMAP frequency bands
• Scalar quadratic maximum likelihood estimators for the CMB cross power spectrum
• Estimation of Full Sky Power Spectrum between Intermediate to Large Angular Scales from Partial Sky CMB Anisotropies using Artificial Neural Network
• A Simulation-Based Method for Correcting Mode Coupling in CMB Angular Power Spectra
• Observing small-scale $\gamma$-ray anisotropies with the Cherenkov Telescope Array
• On the effect of cosmic rays in bolometric CMB measurements from the stratosphere
• Efficient computation of the super-sample covariance for stage IV galaxy surveys
• Characteristic Functions for Cosmological Cross-Correlations
• An Unbiased Estimator of the Full-sky CMB Angular Power Spectrum at Large Scales using Neural Networks
• Accurate estimation of angular power spectra for maps with correlated masks
• Isotropy-Violation Diagnostics for $B$-mode Polarization Foregrounds to the Cosmic Microwave Background
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• Bayesian inference on the sphere beyond statistical isotropy
• Constraining the X-ray AGN halo occupation distribution: implications for eROSITA
• Spatial and Temporal Stability of Airglow Measured in the Meinel Band Window at 1191.3 nm
• The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey
• Optimal strategy for polarization modulation in the LSPE-SWIPE experiment
• Towards efficient and optimal analysis of CMB anisotropies on a masked sky
• Propagating spatially-varying multiplicative shear bias to cosmological parameter estimation for stage-IV weak-lensing surveys
• All-sky angular power spectra from cleaned WISE$\times$SuperCOSMOS galaxy number counts
• Constraints on the SZ Power Spectrum on Degree Angular Scales in WMAP Data
• CMB lensing power spectrum without noise bias
• Science-driven 3D data compression
• General solutions of the leakage in integral transforms and applications to the EB-leakage and detection of the cosmological gravitational wave background
• Estimates of unresolved point sources contribution to WMAP 5
• Clustering properties of the CatWISE2020 quasar catalogue and their impact on the cosmic dipole anomaly
• Partial CMB maps: bias removal and optimal binning of the angular power spectrum
• Measuring the velocity field from type Ia supernovae in an LSST-like sky survey
• COMAP Pathfinder -- Season 2 results II. Updated constraints on the CO(1-0) power spectrum
• On the wavelet analysis of CMB time ordered data: application to Archeops
• The anomaly of the CMB power with the latest Planck data
• Tomographic cross correlations between galaxy surveys and the CMB gravitational lensing potential. Effect of the redshift bin mismatch
• A Bayesian estimate of the CMB-large-scale structure cross-correlation
• On the impact of the galaxy window function on cosmological parameter estimation
• On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
• Masking versus removing point sources in CMB data: the source corrected WMAP power spectrum from new extended catalogue
• How accurately can suborbital experiments measure the CMB?
• WHIM-hunting through cross-correlation of optical and SZ effect data in the Virgo cluster filaments
• Testing Quadratic Maximum Likelihood estimators for forthcoming Stage-IV weak lensing surveys
• The T-E correlation coefficient of Planck legacy data
• A Monte Carlo comparison between template-based and Wiener-filter CMB dipole estimators
• Constraints on primordial non-Gaussianity from Quaia
• Imaging parity-violation in the CMB
• Reconstruction of Missing Data using Iterative Harmonic Expansion
• Effect of noncircularity of experimental beam on CMB parameter estimation
• Expanded Generalized Needlet Internal Linear Combination (eGNILC) Framework for the 21-cm Foreground Removal
• Polarization of Cosmic Microwave Background
• Cross-correlating IceCube neutrinos with a large set of galaxy samples around redshift z ~ 1
• Higher-Order Spectra of Weak Lensing Convergence Maps in Parameterized Theories of Modified Gravity
• Foreground removal from WMAP 7yr polarization maps using an MLP neural network
• The power spectrum of the cosmic microwave background Kolmogorov maps: possible clue to correlation of voids
• The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps
• Constraining cosmic polarization rotation and implications for primordial B-modes
• Cosmic Kite: Auto-encoding the Cosmic Microwave Background
• Effects of boosting on extragalactic components: methods and statistical studies
• CMB likelihood approximation for banded probability distributions
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• The two-and three-point correlation functions of the polarized five-year WMAP sky maps
• The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: III. CMB Temperature Anomalies
• Improved Gibbs samplers for Cosmic Microwave Background power spectrum estimation
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• Foreground removal and angular power spectrum estimation of 21 cm signal using harmonic space ILC method
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: II. Angular Power Spectra and Likelihood
• Goodness--of--fit Statistics and CMB Data Sets
• From top-hat masking to smooth transitions: P-filter and its application to polarized microwave sky maps
• Application of beam deconvolution technique to power spectrum estimation for CMB measurements
• Archeops: an instrument for present and future cosmology
• Needlet estimation of cross-correlation between CMB lensing maps and LSS
• Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
• Optimization of the half wave plate configuration for the LSPE-SWIPE experiment
• Cross-correlating 2MRS galaxies with UHECR flux from Pierre Auger Observatory
• A Modified chi^2-Test for CMB Analyses
• Effect of Fourier filters in removing periodic systematic effects from CMB data
• A Partial-Sky Gibbs ILC Approach for the Estimation of CMB Posterior over Large Angular Scales of the Sky
• A low-rank approach to image defringing
• Galaxy Clustering in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Real-Space Results
• Robust Likelihoods for Inflationary Gravitational Waves from Maps of Cosmic Microwave Background Polarization
• JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium
• Extracting cosmological signals from foregrounds in deep mm maps of the sky
• Cosmological Parameter Estimation: Method
• Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times 2$pt Photometric Survey
• Spectrum of radiation from global strings and the relic axion density
• An update on Archeops: flights and data products
• KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays
• Pixel domain multi-resolution minimum variance painting of CMB maps
• Improved Method for Detecting Local Discontinuities in CMB data by Finite Differencing
• Cross-correlating the EMU Pilot Survey 1 with CMB lensing: Constraints on cosmology and galaxy bias with harmonic-space power spectra
• A Search for X-Ray Reionization Signatures from Cross-Correlation of Wmap and ROSAT Rass Data
• Optimal map-making with singularities
• Fast computation of temperature and polarization coupling matrices
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• Reconstructing the shape of the correlation function
• Local bandpower diagnostics for the hemispherical power asymmetry in CMB E-mode polarization
• FuGa3D: Fast full-sky analysis of Galaxy catalogs in 3D
• On the detection of point sources in Planck LFI 70 GHz CMB maps based on cleaned K-map
• Detectability of Galactic Faraday Rotation in Multi-wavelength CMB Observations: A Cross-Correlation Analysis of CMB and Radio Maps
• Euclid: Optimising tomographic redshift binning for 3$\times$2pt power spectrum constraints on dark energy
• Primordial non-Gaussianity systematics from redshift mismatch with SPHEREx
• The Parameter-Level Performance of Covariance Matrix Conditioning in Cosmic Microwave Background Data Analyses
• CMB lensing tomography with clustering estimation of lens redshift distributions
• Large-scale Modeling of the Observed Power Spectrum Multipoles
• The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations
• Skew-spectra: a generalization to spin-$s$
• Systematics mitigation for catalogue-based angular power spectra
• Constraining Quintessence Models with ISW-tSZ Cross-Correlations: A Comparative Analysis of Thawing, Tracker, and Scaling-Freezing Dynamics