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Record W4402823334 · doi:10.48550/arxiv.2409.02296

Development of the 220/270 GHz Receiver of BICEP Array

2024· preprint· en· W4402823334 on OpenAlexaff
Y. Nakato, Zafar U. Ahmed, Mojtaba Amiri, D. Barkats, R. Basu Thakur, D. Beck, V. Buza, B Cantrall, J. Cornelison, M. Crumrine, Edward Denison, M. Dierickx, L. Duband, M. Eiben, S. Fatigoni, Antonio Fortes, Maocheng Gao, Christos Giannakopoulos, N. Goeckner-Wald, G. Hall, George Halal, Manfred Halpern, E. Hand, Steven J. Harrison, S. Henderson, Johannes Hubmayr, H. Hui, Jing X. Kang, E. Karpel, S. Kefeli, K. Lau, Margaret Lautzenhiser, A. Lennox, Tong Liu, M. Catherine Miller, Lorenzo Minutolo, Lorenzo Moncelsi, R. O’Brient, Aniruddh D. Patel, M Petroff, T. Prouvé, C. Pryke, T. Romand, Maria Salatino, A. Schillaci, B Singari, Adel S. Soliman, A. Steiger, B. Steinbach, R. Sudiwala, C. Tucker, C. Vergès, A. Wandui, J. Willmert, H. Yang, Edward Young, Cyndia Yu, Linwei Zeng, Chun‐Dong Zhang, S. Zhang

Bibliographic record

VenuearXiv (Cornell University) · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicSuperconducting and THz Device Technology
Canadian institutionsUniversity of British Columbia
FundersSLAC National Accelerator LaboratoryU.S. Department of EnergyW. M. Keck FoundationOffice of ScienceNational Aeronautics and Space AdministrationHarvard UniversityNational Science Foundation
KeywordsComputer scienceTelecommunications

Abstract

fetched live from OpenAlex

Measurements of B-mode polarization in the CMB sourced from primordial gravitational waves would provide information on the energy scale of inflation and its potential form. To achieve these goals, one must carefully characterize the Galactic foregrounds, which can be distinguished from the CMB by conducting measurements at multiple frequencies. BICEP Array is the latest-generation multi-frequency instrument of the BICEP/Keck program, which specifically targets degree-scale primordial B-modes in the CMB. In its final configuration, this telescope will consist of four small-aperture receivers, spanning frequency bands from 30 to 270 GHz. The 220/270 GHz receiver designed to characterize Galactic dust is currently undergoing commissioning at Stanford University and is scheduled to deploy to the South Pole during the 2024--2025 austral summer. Here, we will provide an overview of this high-frequency receiver and discuss the integration status and test results as it is being commissioned.

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)0.002
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.006
Threshold uncertainty score0.020

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0060.006

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 head0.059
GPT teacher head0.192
Teacher spread0.133 · 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 designBench or experimental
Domainnot available
GenreEmpirical

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

Citations0
Published2024
Admission routes1
Has abstractyes

Explore more

Same venuearXiv (Cornell University)→Same topicSuperconducting and THz Device Technology→French-language works237,207→