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Record W2789053168 · doi:10.1088/1538-3873/aab0fe

A Binary Offset Effect in CCD Readout and Its Impact on Astronomical Data

2018· article· en· W2789053168 on OpenAlex
K. Boone, G. Aldering, Y. Copin, S. Dixon, R. S. Domagalski, É. Gangler, É. Pécontal, S. Perlmutter

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.
fundA Canadian funder is recorded on the work.

Bibliographic record

VenuePublications of the Astronomical Society of the Pacific · 2018
Typearticle
Languageen
FieldEngineering
TopicCCD and CMOS Imaging Sensors
Canadian institutionsUniversity of Toronto
FundersSLAC National Accelerator LaboratoryLawrence Berkeley National LaboratoryComisión Nacional de Investigación Científica y TecnológicaArgonne National LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityInstitut National de Physique Nucléaire et de Physique des ParticulesYork UniversityMinistério da Ciência, Tecnologia e InovaçãoScience and Technology Facilities CouncilOffice of ScienceUniversity of Illinois at Urbana-ChampaignSpace Telescope Science InstituteUniversity of SussexInstitut de Física d'Altes EnergiesU.S. Department of EnergyYale UniversityFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoCentre National de la Recherche ScientifiqueBrookhaven National LaboratoryHigh Energy PhysicsDeutsche ForschungsgemeinschaftMinisterio de Ciencia, Tecnología e Innovación ProductivaNational Aeronautics and Space AdministrationUniversity College LondonCarnegie Mellon UniversityCollege of Engineering, Michigan State UniversityUniversity of WashingtonAlfred P. Sloan FoundationNASA Exoplanet Science InstitutePrinceton UniversityJohns Hopkins UniversityInstitut national des sciences de l'UniversVanderbilt UniversityUniversity of ChicagoHarvard UniversityAgence Nationale de la RechercheOhio State UniversityFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaNational Astronomical Observatory of JapanNew Mexico State UniversityUniversity of PortsmouthGordon and Betty Moore FoundationCalifornia Institute of TechnologyAdvanced Scientific Computing ResearchW. M. Keck FoundationFermilabNational Science Foundation
KeywordsPixelTelescopePhysicsOffset (computer science)Binary numberDigitizationOpticsData reductionRemote sensingAstronomyAstrophysicsComputer scienceTelecommunicationsGeology

Abstract

fetched live from OpenAlex

We have discovered an anomalous behavior of CCD readout electronics that affects their use in many astronomical applications. An offset in the digitization of the CCD output voltage that depends on the binary encoding of one pixel is added to pixels that are read out one, two, and/or three pixels later. One result of this effect is the introduction of a differential offset in the background when comparing regions with and without flux from science targets. Conventional data reduction methods do not correct for this offset. We find this effect in 16 of 22 instruments investigated, covering a variety of telescopes and many different front-end electronics systems. The affected instruments include LRIS and DEIMOS on the Keck telescopes, WFC3 UVIS and STIS on HST , MegaCam on CFHT, SNIFS on the UH88 telescope, GMOS on the Gemini telescopes, HSC on Subaru, and FORS on VLT. The amplitude of the introduced offset is up to 4.5 ADU per pixel, and it is not directly proportional to the measured ADU level. We have developed a model that can be used to detect this “binary offset effect” in data, and correct for it. Understanding how data are affected and applying a correction for the effect is essential for precise astronomical measurements.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.156
Threshold uncertainty score0.361

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 science0.0010.000
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 head0.014
GPT teacher head0.255
Teacher spread0.241 · 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