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Record W2997120571 · doi:10.2514/6.2020-1595

Composite Magnitude: A tool for creating better star tracker catalogs

2020· article· en· W2997120571 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.

Bibliographic record

VenueAIAA Scitech 2020 Forum · 2020
Typearticle
Languageen
FieldEngineering
TopicInertial Sensor and Navigation
Canadian institutionsToronto Metropolitan University
Fundersnot available
KeywordsStar trackerBrightnessMagnitude (astronomy)StarsPhysicsGuide starStar (game theory)Apparent magnitudeComputer scienceDetectorMetric (unit)CalibrationEclipseComputer visionArtificial intelligenceAstrophysicsOpticsAstronomy

Abstract

fetched live from OpenAlex

This paper presents a process for building star tracker star catalogs with the aim of improving photometric predictability, reducing the required number of calibration images, and increasing the sensor availability. We introduce a technique to predict the apparent brightness of stars as perceived by imaging optical sensors such as star trackers. This prediction method uses a small set of reference stars with average measured brightness to estimate the apparent brightness of all other stars. This approach relies on the calculation of a brightness metric called composite magnitude. This metric is similar to visual magnitude but also incorporates the photometric responses of the star in the UBVRI Johnson-Cousins system, optical properties of the star tracker lens, and the quantum efficiency of the pixel detector. Furthermore, we can use the method presented to predict performance of the star catalogs when lens or detector properties are modified during the star tracker development. The presented brightness prediction technique is validated by on-orbit and ground test telemetry data.

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.

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 score0.464
Threshold uncertainty score0.694

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 head0.008
GPT teacher head0.214
Teacher spread0.206 · 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