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Record W3151173739 · doi:10.3847/1538-4357/ac230b

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

2021· preprint· en· W3151173739 on OpenAlexfundno aff
A. E. Gambrel, A. Rahlin, Xue Song, Carlo Contaldi, P. A. R. Ade, M. Amiri, S. J. Benton, A. S. Bergman, R. Bihary, J. J. Bock, J. Richard Bond, J. A. Bonetti, Sean Bryan, H. C. Chiang, Adriaan J. Duivenvoorden, H. K. Eriksen, M. Farhang, J. P. Filippini, A. A. Fraisse, Katherine Freese, M. Galloway, N. N. Gandilo, R. Gualtieri, Jon E. Gudmundsson, M. Halpern, John W. Hartley, Matthew Hasselfield, G. C. Hilton, W. Holmes, V. V. Hristov, Zhiqi Huang, K. D. Irwin, W. C. Jones, A. Karakci, C. L. Kuo, Z. Kermish, Jason S.-Y. Leung, Lun Li, D. S. Y. Mak, P. Mason, K. G. Megerian, Lorenzo Moncelsi, T. A. Morford, Johanna M. Nagy, C. B. Netterfield, M. R. Nolta, R. O’Brient, B. Osherson, Ivan L. Padilla, B. Racine, C. D. Reintsema, J. E. Ruhl, T. M. Ruud, J. A. Shariff, E. C. Shaw, Corwin Shiu, J. D. Soler, A. Trangsrud, C. Tucker, R. S. Tucker, Anthony Turner, J. F. van der List, A. C. Weber, I. K. Wehus, S. Wen, Donald Wiebe, E. Young

Bibliographic record

VenueThe Astrophysical Journal · 2021
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsnot available
FundersBritish Antarctic SurveyBritish Columbia Knowledge Development FundNorges ForskningsrådScience and Technology Facilities CouncilUniversity of TorontoCanadian Space AgencyInyuvesi Yakwazulu-NataliUK Research and InnovationUniversity of Texas at AustinPrinceton UniversityScience Mission DirectorateGovernment of OntarioNational Aeronautics and Space AdministrationNational Science FoundationCompute CanadaUniversity of ChicagoVetenskapsrådet
KeywordsEstimatorMonte Carlo methodCosmic microwave backgroundAlgorithmPlanckMarkov chain Monte CarloPhysicsSpectral densityHybrid Monte CarloStatistical physicsComputer scienceStatisticsAstrophysicsMathematicsAnisotropyOptics

Abstract

fetched live from OpenAlex

Abstract We present the XFaster analysis package, a fast, iterative angular power spectrum estimator based on a diagonal approximation to the quadratic Fisher matrix estimator. It uses Monte Carlo simulations to compute noise biases and filter transfer functions and is thus a hybrid of both Monte Carlo and quadratic estimator methods. In contrast to conventional pseudo-C ℓ –based methods, the algorithm described here requires a minimal number of simulations and does not require them to be precisely representative of the data to estimate accurate covariance matrices for the bandpowers. The formalism works with polarization-sensitive observations and also data sets with identical, partially overlapping, or independent survey regions. The method was first implemented for the analysis of BOOMERanG data and also used as part of the Planck analysis. Here we describe the full, publicly available analysis package, written in Python, as developed for the analysis of data from the 2015 flight of the Spider instrument. The package includes extensions for self-consistently estimating null spectra and estimating fits for Galactic foreground contributions. We show results from the extensive validation of XFaster using simulations and its application to the Spider data set.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.003
metaresearch head score (Gemma)0.019
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Methods · Consensus signal: Methods
Teacher disagreement score0.008
Threshold uncertainty score0.027

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.019
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.001
Science and technology studies0.0000.001
Scholarly communication0.0010.002
Open science0.0020.002
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0080.002

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.010
GPT teacher head0.259
Teacher spread0.249 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreMethods

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations1
Published2021
Admission routes1
Has abstractyes

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