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Record W4408697246 · doi:10.1117/12.3061924

Star tracker algorithm improvements to restore performance after radiation exposure

2025· article· en· W4408697246 on OpenAlexaff
Abigail Lee

Bibliographic record

Venuenot available
Typearticle
Languageen
FieldEngineering
TopicInertial Sensor and Navigation
Canadian institutionsQueen's University
Fundersnot available
KeywordsComputer scienceStar (game theory)Star trackerAlgorithmArtificial intelligencePhysicsAstronomyAstrophysics

Abstract

fetched live from OpenAlex

Rocket Lab’s ST16-RT2 star tracker uses a CMOS detector to image stars in the sensor’s field of view, software to isolate the stars in the image from the background, and an on-board catalogue to identify the stars in the image and, thus, determine the attitude of the satellite. High temperatures and radiation effects raise the black level and standard deviation of the noise on the sensor. This results in a loss of dynamic range and complicates the pixel classification between star candidates and the background. Pixels improperly designated as part of a star are referred to as false positives, and pixels improperly designated as the background are false negatives. A high quantity of false positives adds to the processing time required to identify stars in an image and has the potential to reduce the accuracy of the attitude solutions provided by the star tracker. To maximize the dynamic range available to a specific sensor, Rocket Lab calibrates analog offsets to the device at room temperature. In higher temperature and radiation environments, the star tracker’s dynamic range is reduced and background noise increases. This increases the quantity of false-positive pixels which, in turn, limits star tracker performance. Utilizing analog offsets determined on-chip and a more robust thresholding algorithm, the star tracker can recover dynamic range and more effectively suppress noise. Such improvements would extend a star tracker's life or allow the product to be used in more extreme environments, without compromising the hardware heritage. To implement these improvements, the limitations of the current thresholding algorithm were analyzed, and a new algorithm was developed. Dark image data was collected using non-irradiated and irradiated detectors, with both the preset and on-chip analog offsets, at temperatures ranging from 20 °C to 70 °C. Processing the dark images using this new approach showed a significant reduction in false-positive pixels recorded using the irradiated boards compared to the current algorithm. The reduction in false positives prevented the lit pixel buffer from filling until 64°C, a 30 °C increase in performance for the irradiated boards. Images were then collected using simulated star fields at various slew rates to determine if the reduction in false positives led to an increase in false negatives. Thresholding parameters were tuned and recommended configurations were given for on-orbit testing.

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)0.006
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: Empirical · Consensus signal: none
Teacher disagreement score0.008
Threshold uncertainty score0.027

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.006
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0020.002
Open science0.0020.001
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0080.006

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 head0.003
GPT teacher head0.199
Teacher spread0.196 · 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
Published2025
Admission routes1
Has abstractyes

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