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Record W2884926209 · doi:10.1117/12.2312942

Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

2018· preprint· en· W2884926209 on OpenAlexaff
Ahmed Soliman, Steve J. Benton, Colin A. Bischoff, James J. Bock, E. Bullock, Cora Dvorkin, Jeff P. Filippini, S. Fliescher, J. Grayson, Mark Halpern, Sam A. Harrison, S. R. Hildebrandt, Gene Hilton, H. Hui, K. D. Irwin, J. Kang, Kirit S. Karkare, E. Karpel, Jonathan Kaufman, Brian Keating, Sinan Kefeli, Sarah A. Kernasovskiy, J. M. Kovac, Chao‐Lin Kuo, Nicole Larson, K. Lau, E. M. Leitch, M. Lueker, K. G. Megerian, Lorenzo Moncelsi, Toshiya Namikawa, C. B. Netterfield, H. T. Nguyen, Roger O’Brient, R. W. Ogburn, Stephen Palladino, C. Pryke, B. Racine, S. Richter, A. Schillaci, Robert Schwarz, Abigail G. Vieregg, A. Wandui, Alexis C. Weber, Don Wiebe, Justin Willmert, Chin Lin Wong, Wai Ling K. Wu, Hung-I E. Yang, K. W. Yoon, Cheng Zhang, P. A. R. Ade, Zeeshan Ahmed, R. Aikin, Kate D. Alexander, D. Barkats, Rachel Bowens-Rubin, Justus A. Brevik, I. Buder, V. Buza, J. Cornelison, B. P. Crill, M. Crumrine, M. Dierickx, L. Duband, Grantland Hall, Chris D. Sheehy, T. St. Germaine, Z. Staniszewski, B. Steinbach, R. Sudiwala, G. P. Teply, K. L. Thompson, J. E. Tolan, C. Tucker, Anthony Turner, Caterina Umiltà, Jakob J. Vanzyl

Bibliographic record

Venuenot available
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsUniversity of Toronto
FundersSLAC National Accelerator LaboratoryHarvard UniversityOffice of ScienceNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyGordon and Betty Moore FoundationW. M. Keck FoundationAdvanced Research Projects AgencyNational Science Foundation
KeywordsDetectorPhysicsCosmic microwave backgroundPolarization (electrochemistry)Bandwidth (computing)MicrowaveOpticsBeam (structure)Computer scienceTelecommunications

Abstract

fetched live from OpenAlex

BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad frequency range with channels at 30/40, 95, 150 and 220/270 GHz. The first low-frequency receiver will map synchrotron emission at 30 and 40 GHz and will deploy to the South Pole at the end of 2019. In this paper, we give an overview of the BICEP Array science and instrument, with a focus on the detector module. We designed corrugations in the metal frame of the module to suppress unwanted interactions with the antenna-coupled detectors that would otherwise deform the beams of edge pixels. This design reduces the residual beam systematics and temperature-to-polarization leakage due to beam steering and shape mismatch between polarized beam pairs. We report on the simulated performance of single- and wide-band corrugations designed to minimize these effects. Our optimized design alleviates beam differential ellipticity caused by the metal frame to about 7% over 57% bandwidth (25 to 45 GHz), which is close to the level due the bare antenna itself without a metal frame. Initial laboratory measurements are also presented.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.670
Threshold uncertainty score0.810

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.021
GPT teacher head0.225
Teacher spread0.204 · 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 teacher head, 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

Citations12
Published2018
Admission routes1
Has abstractyes

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