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Record W3208331988 · doi:10.1093/mnras/stac130

Realistic galaxy image simulation via score-based generative models

2022· preprint· en· W3208331988 on OpenAlex
Michael J. Smith, J. E. Geach, R. A. JACKSON, Nikhil Arora, Connor Stone, Stéphane Courteau

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

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typepreprint
Languageen
FieldComputer Science
TopicGenerative Adversarial Networks and Image Synthesis
Canadian institutionsQueen's University
FundersArgonne National LaboratoryScience and Technology Facilities CouncilJet Propulsion LaboratoryUniversity of Illinois at Urbana-ChampaignSLAC National Accelerator LaboratoryQueen's UniversityChinese Academy of SciencesU.S. Department of EnergyNational Natural Science Foundation of ChinaDeutsche ForschungsgemeinschaftUniversity of PortsmouthUniversity of HertfordshireOffice of ScienceUniversity of EdinburghConsejo Superior de Investigaciones CientíficasCenter for Cosmology and Astroparticle Physics, Ohio State UniversityNational Research Foundation of KoreaUniversity of SussexNational Aeronautics and Space AdministrationUniversity College LondonEidgenössische Technische Hochschule ZürichNational Centre for Supercomputing ApplicationsTexas A and M UniversityUniversity of ChicagoOhio State UniversityCalifornia Institute of TechnologyHigher Education Funding Council for EnglandLawrence Berkeley National LaboratoryDivision of Astronomical SciencesFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaUniversity of NottinghamStanford UniversityNatural Sciences and Engineering Research Council of CanadaYonsei UniversityUniversity of MichiganRoyal SocietyNational Science Foundation
KeywordsGalaxyComputer scienceSkyInferenceArtificial intelligenceSimilarity (geometry)Ground truthPhysicsAstrophysicsImage (mathematics)

Abstract

fetched live from OpenAlex

ABSTRACT We show that a denoising diffusion probabilistic model (DDPM), a class of score-based generative model, can be used to produce realistic mock images that mimic observations of galaxies. Our method is tested with Dark Energy Spectroscopic Instrument (DESI) grz imaging of galaxies from the Photometry and Rotation curve OBservations from Extragalactic Surveys (PROBES) sample and galaxies selected from the Sloan Digital Sky Survey. Subjectively, the generated galaxies are highly realistic when compared with samples from the real data set. We quantify the similarity by borrowing from the deep generative learning literature, using the ‘Fréchet inception distance’ to test for subjective and morphological similarity. We also introduce the ‘synthetic galaxy distance’ metric to compare the emergent physical properties (such as total magnitude, colour, and half-light radius) of a ground truth parent and synthesized child data set. We argue that the DDPM approach produces sharper and more realistic images than other generative methods such as adversarial networks (with the downside of more costly inference), and could be used to produce large samples of synthetic observations tailored to a specific imaging survey. We demonstrate two potential uses of the DDPM: (1) accurate inpainting of occluded data, such as satellite trails, and (2) domain transfer, where new input images can be processed to mimic the properties of the DDPM training set. Here we ‘DESI-fy’ cartoon images as a proof of concept for domain transfer. Finally, we suggest potential applications for score-based approaches that could motivate further research on this topic within the astronomical community.

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)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Methods · Consensus signal: none
Teacher disagreement score0.745
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0020.003
Research integrity0.0000.001
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 head0.021
GPT teacher head0.233
Teacher spread0.212 · 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