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Record W3023795130 · doi:10.1051/0004-6361/202038219

HOLISMOKES

2020· article· en· W3023795130 on OpenAlexfundno aff

Bibliographic record

VenueAstronomy and Astrophysics · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersPlanetary Science DivisionJapan Society for the Promotion of ScienceSmithsonian Astrophysical ObservatoryUniversity of EdinburghMax-Planck-Institut für AstronomieNational Astronomical Observatory of JapanMax-Planck-GesellschaftMinistry of Education, Culture, Sports, Science and TechnologyQueen's UniversityCabinet Office, Government of JapanScience Mission DirectorateSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungSpace Telescope Science InstituteToray Science FoundationUniversity of TokyoHigh Energy Accelerator Research OrganizationEötvös Loránd TudományegyetemAcademia SinicaEuropean CommissionLos Alamos National LaboratoryJohns Hopkins UniversityPrinceton UniversityNational Central UniversityGordon and Betty Moore FoundationQueen's University BelfastNational Aeronautics and Space AdministrationDurham UniversityJapan Science and Technology AgencySmithsonian InstitutionNational Science Foundation
KeywordsGalaxyLens (geology)RedshiftSkyConvolutional neural networkPhotometry (optics)SupernovaVelocity dispersion

Abstract

fetched live from OpenAlex

We present a systematic search for wide-separation (with Einstein radiusθE ≳ 1.5″), galaxy-scale strong lenses in the 30 000 deg2of the Pan-STARRS 3πsurvey on the Northern sky. With long time delays of a few days to weeks, these types of systems are particularly well-suited for catching strongly lensed supernovae with spatially-resolved multiple images and offer new insights on early-phase supernova spectroscopy and cosmography. We produced a set of realistic simulations by painting lensed COSMOS sources on Pan-STARRS image cutouts of lens luminous red galaxies (LRGs) with redshift and velocity dispersion known from the sloan digital sky survey (SDSS). First, we computed the photometry of mock lenses ingribands and applied a simple catalog-level neural network to identify a sample of 1 050 207 galaxies with similar colors and magnitudes as the mocks. Second, we trained a convolutional neural network (CNN) on Pan-STARRSgriimage cutouts to classify this sample and obtain sets of 105 760 and 12 382 lens candidates with scores ofpCNN > 0.5 and > 0.9, respectively. Extensive tests showed that CNN performances rely heavily on the design of lens simulations and the choice of negative examples for training, but little on the network architecture. The CNN correctly classified 14 out of 16 test lenses, which are previously confirmed lens systems above the detection limit of Pan-STARRS. Finally, we visually inspected all galaxies withpCNN > 0.9 to assemble a final set of 330 high-quality newly-discovered lens candidates while recovering 23 published systems. For a subset, SDSS spectroscopy on the lens central regions proves that our method correctly identifies lens LRGs atz ∼ 0.1–0.7. Five spectra also show robust signatures of high-redshift background sources, and Pan-STARRS imaging confirms one of them as a quadruply-imaged red source atzs = 1.185, which is likely a recently quenched galaxy strongly lensed by a foreground LRG atzd = 0.3155. In the future, high-resolution imaging and spectroscopic follow-up will be required to validate Pan-STARRS lens candidates and derive strong lensing models. We also expect that the efficient and automated two-step classification method presented in this paper will be applicable to the ∼4 mag deepergristacks from theRubinObservatory Legacy Survey of Space and Time (LSST) with minor adjustments.

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)0.003
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.392
Threshold uncertainty score0.000

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.002
Science and technology studies0.0020.001
Scholarly communication0.0050.006
Open science0.0010.004
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.3920.178

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 head0.009
GPT teacher head0.192
Teacher spread0.183 · 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 designObservational
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

Citations72
Published2020
Admission routes1
Has abstractyes

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