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Record W4405831008 · doi:10.1117/1.jatis.10.4.044012

In-flight performance of Spider’s 280-GHz receivers

2024· article· en· W4405831008 on OpenAlexaff
Elle C. Shaw, Peter A. R. Ade, Scott Akers, M. Amiri, Jason E. Austermann, James A. Beall, Daniel Becker, Steven J. Benton, A. S. Bergman, James J. Bock, J. Richard Bond, Sean Bryan, H. C. Chiang, Carlo Contaldi, R. S. Domagalski, Olivier Doré, Shannon M. Duff, Adriaan J. Duivenvoorden, Hans K. Eriksen, J. P. Filippini, L. M. Fissel, Aurélien A. Fraisse, Katherine Freese, M. Galloway, A. E. Gambrel, N. N. Gandilo, K. Ganga, Sho M. Gibbs, Suren Gourapura, Arpi Grigorian, R. Gualtieri, Mark Halpern, John Hartley, Matthew Hasselfield, Gene Hilton, Warren Holmes, Viktor Hristov, Zhiqi Huang, Johannes Hubmayr, K. D. Irwin, William C. Jones, Asad Kahn, Z. Kermish, Cesiley King, C.-L. Kuo, Amber R. Lennox, Jason S.-Y. Leung, Steven Li, Thuy Vy T. Luu, P. Mason, Jared May, Krikor G. Megerian, Lorenzo Moncelsi, T. A. Morford, Johanna M. Nagy, Rong Nie, Calvin B. Netterfield, Michael R. Nolta, B. Osherson, Ivan L. Padilla, A. Rahlin, Susan F. Redmond, Carl Reintsema, L. Javier Romualdez, J. E. Ruhl, Marcus C. Runyan, J. A. Shariff, Corwin Shiu, J. D. Soler, Xue Song, Simon Tartakovsky, H. Thommesen, A. Trangsrud, C. Tucker, Anthony D. Turner, Joel Ullom, J. F. van der List, Jeff Van Lanen, Michael R. Vissers, Alexis C. Weber, I. K. Wehus, Shyang Wen, Donald Wiebe, E. Young

Bibliographic record

VenueJournal of Astronomical Telescopes Instruments and Systems · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoQueen's UniversityMcGill UniversityUniversity of British Columbia
Fundersnot available
KeywordsSkySpiderCosmic microwave backgroundRemote sensingPhysicsDetectorRangingGravitational waveMicrowaveStratosphereAstronomyOpticsMeteorologyGeologyGeodesy

Abstract

fetched live from OpenAlex

Spider is a balloon-borne instrument designed to map the cosmic microwave background at degree-angular scales in the presence of Galactic foregrounds. Spider has mapped a large sky area in the Southern Hemisphere using more than 2000 transition-edge sensors (TESs) during two NASA Long Duration Balloon flights above the Antarctic continent. During its first flight in January 2015, Spider was observed in the 95- and 150-GHz frequency bands, setting constraints on the B-mode signature of primordial gravitational waves. Its second flight in the 2022–2023 season added new receivers at 280 GHz, each using an array of TESs coupled to the sky through feedhorns formed from stacks of silicon wafers. These receivers are optimized to produce deep maps of polarized Galactic dust emission over a large sky area, providing a unique data set with lasting value to the field. We describe the instrument’s performance during Spider’s second flight, focusing on the performance of the 280-GHz receivers. We include details on the flight, in-band optical loading at float, and an early analysis of detector noise.

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)0.001
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: Empirical
Teacher disagreement score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0000.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0020.001

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 head0.235
Teacher spread0.225 · 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

Citations1
Published2024
Admission routes1
Has abstractyes

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