Marginal unbiased score expansion and application to CMB lensing

Here, we present the marginal unbiased score expansion (MUSE) method, an algorithm for generic high-dimensional hierarchical Bayesian inference. MUSE performs approximate marginalization over arbitrary non-Gaussian latent parameter spaces, yielding Gaussianized asymptotically unbiased and near-optim...

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Published in:Physical Review D
Main Authors: Millea, Marius, Seljak, Uroš
Language:unknown
Published: 2023
Subjects:
Online Access:http://www.osti.gov/servlets/purl/1878325
https://www.osti.gov/biblio/1878325
https://doi.org/10.1103/physrevd.105.103531
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spelling ftosti:oai:osti.gov:1878325 2023-07-30T04:06:55+02:00 Marginal unbiased score expansion and application to CMB lensing Millea, Marius Seljak, Uroš 2023-05-25 application/pdf http://www.osti.gov/servlets/purl/1878325 https://www.osti.gov/biblio/1878325 https://doi.org/10.1103/physrevd.105.103531 unknown http://www.osti.gov/servlets/purl/1878325 https://www.osti.gov/biblio/1878325 https://doi.org/10.1103/physrevd.105.103531 doi:10.1103/physrevd.105.103531 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS 2023 ftosti https://doi.org/10.1103/physrevd.105.103531 2023-07-11T10:13:45Z Here, we present the marginal unbiased score expansion (MUSE) method, an algorithm for generic high-dimensional hierarchical Bayesian inference. MUSE performs approximate marginalization over arbitrary non-Gaussian latent parameter spaces, yielding Gaussianized asymptotically unbiased and near-optimal constraints on global parameters of interest. It is computationally much cheaper than exact alternatives like Hamiltonian Monte Carlo (HMC), excelling on funnel problems which challenge HMC, and does not require any problem-specific user supervision like other approximate methods such as variational inference or many simulation-based inference methods. MUSE makes possible the first joint Bayesian estimation of the delensed Cosmic Microwave Background (CMB) power spectrum and gravitational lensing potential power spectrum, demonstrated here on a simulated data set as large as the upcoming South Pole Telescope 3G 1500 deg 2 survey, corresponding to a latent dimensionality of ~6 million and of order 100 global bandpower parameters. On a subset of the problem where an exact but more expensive HMC solution is feasible, we verify that MUSE yields nearly optimal results. We also demonstrate that existing spectrum-based forecasting tools which ignore pixel-masking underestimate predicted error bars by only ~10%. This method is a promising path forward for fast lensing and delensing analyses which will be necessary for future CMB experiments such as SPT-3G, Simons Observatory, or CMB-S4, and can complement or supersede existing HMC approaches. The success of MUSE on this challenging problem strengthens its case as a generic procedure for a broad class of high-dimensional inference problems. Other/Unknown Material South pole SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy) South Pole Physical Review D 105 10
institution Open Polar
collection SciTec Connect (Office of Scientific and Technical Information - OSTI, U.S. Department of Energy)
op_collection_id ftosti
language unknown
topic 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
spellingShingle 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Millea, Marius
Seljak, Uroš
Marginal unbiased score expansion and application to CMB lensing
topic_facet 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
description Here, we present the marginal unbiased score expansion (MUSE) method, an algorithm for generic high-dimensional hierarchical Bayesian inference. MUSE performs approximate marginalization over arbitrary non-Gaussian latent parameter spaces, yielding Gaussianized asymptotically unbiased and near-optimal constraints on global parameters of interest. It is computationally much cheaper than exact alternatives like Hamiltonian Monte Carlo (HMC), excelling on funnel problems which challenge HMC, and does not require any problem-specific user supervision like other approximate methods such as variational inference or many simulation-based inference methods. MUSE makes possible the first joint Bayesian estimation of the delensed Cosmic Microwave Background (CMB) power spectrum and gravitational lensing potential power spectrum, demonstrated here on a simulated data set as large as the upcoming South Pole Telescope 3G 1500 deg 2 survey, corresponding to a latent dimensionality of ~6 million and of order 100 global bandpower parameters. On a subset of the problem where an exact but more expensive HMC solution is feasible, we verify that MUSE yields nearly optimal results. We also demonstrate that existing spectrum-based forecasting tools which ignore pixel-masking underestimate predicted error bars by only ~10%. This method is a promising path forward for fast lensing and delensing analyses which will be necessary for future CMB experiments such as SPT-3G, Simons Observatory, or CMB-S4, and can complement or supersede existing HMC approaches. The success of MUSE on this challenging problem strengthens its case as a generic procedure for a broad class of high-dimensional inference problems.
author Millea, Marius
Seljak, Uroš
author_facet Millea, Marius
Seljak, Uroš
author_sort Millea, Marius
title Marginal unbiased score expansion and application to CMB lensing
title_short Marginal unbiased score expansion and application to CMB lensing
title_full Marginal unbiased score expansion and application to CMB lensing
title_fullStr Marginal unbiased score expansion and application to CMB lensing
title_full_unstemmed Marginal unbiased score expansion and application to CMB lensing
title_sort marginal unbiased score expansion and application to cmb lensing
publishDate 2023
url http://www.osti.gov/servlets/purl/1878325
https://www.osti.gov/biblio/1878325
https://doi.org/10.1103/physrevd.105.103531
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op_relation http://www.osti.gov/servlets/purl/1878325
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doi:10.1103/physrevd.105.103531
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container_title Physical Review D
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