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Record W4319593716 · doi:10.1088/1538-3873/acaebd

The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. IV. Aperture Masking Interferometry

2023· article· en· W4319593716 on OpenAlexafffund
Anand Sivaramakrishnan, Peter Tuthill, James P. Lloyd, Alexandra Z. Greenbaum, Deepashri Thatte, Rachel Cooper, Thomas Vandal, Jens Kammerer, J. Sánchez-Bermúdez, Benjamin Pope, Dori Blakely, Loïc Albert, Neil J. Cook, Doug Johnstone, A. R. Martel, Kevin Volk, A. Soulain, Étienne Artigau, David Lafreniére, Chris J. Willott, Sébastien Parmentier, K. E. Saavik Ford, Barry McKernan, M. Begoña Vila, Neil Rowlands, René Doyon, Mathilde Beaulieu, Louis Desdoigts, A. W. Fullerton, Matthew De Furio, Paul Goudfrooij, S. T. Holfeltz, Stephanie LaMassa, Michael Maszkiewicz, Michael R. Meyer, Marshall D. Perrin, Laurent Pueyo, J. Sahlmann, Sangmo Tony Sohn, P. S. Teixeira, Sheng-Hai Zheng

Bibliographic record

VenuePublications of the Astronomical Society of the Pacific · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsHoneywell (Canada)Herzberg Institute of AstrophysicsCanadian Space AgencyUniversity of VictoriaUniversité de Montréal
FundersNational Aeronautics and Space AdministrationCanadian Space AgencySpace Telescope Science InstituteNational Science Foundation
KeywordsSpectrographPhysicsInterferometryOpticsMasking (illustration)TelescopeAstronomyJames Webb Space TelescopeInfraredSpitzer Space TelescopeAperture (computer memory)Remote sensingGeologySpectral lineArt

Abstract

fetched live from OpenAlex

Abstract The James Webb Space Telescope’s Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, operating at 3–5 μm wavelengths, and a bright limit of ≃4 mag in W2. We describe the NIRISS Aperture Masking Interferometry (AMI) mode to help potential observers understand its underlying principles, present some sample science cases, explain its operational observing strategies, indicate how AMI proposals can be developed with data simulations, and how AMI data can be analyzed. We also present key results from commissioning AMI. Since the allied Kernel Phase Imaging (KPI) technique benefits from AMI operational strategies, we also cover NIRISS KPI methods and analysis techniques, including a new user-friendly KPI pipeline. The NIRISS KPI bright limit is ≃8 W2 (4.6 μm) magnitudes. AMI NRM and KPI achieve an inner working angle of ∼70 mas, which is well inside the ∼400 mas NIRCam inner working angle for its circular occulter coronagraphs at comparable wavelengths.

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: none
GenreCandidate signal: Methods · Consensus signal: Methods
Teacher disagreement score0.009
Threshold uncertainty score0.031

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0090.005

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 head0.223
Teacher spread0.213 · 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
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

Citations22
Published2023
Admission routes2
Has abstractyes

Explore more

Same venuePublications of the Astronomical Society of the PacificSame topicStellar, planetary, and galactic studiesFrench-language works237,207