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Record W4404307610 · doi:10.1051/0004-6361/202452361

PICZL: Image-based photometric redshifts for AGN

2024· article· en· W4404307610 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.

fundA Canadian funder is recorded on the work.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldEngineering
TopicSatellite Image Processing and Photogrammetry
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryArgonne National LaboratoryHigh Energy PhysicsDivision of Astronomical SciencesRussian Academy of SciencesLeibniz-GemeinschaftSmithsonian Astrophysical ObservatoryOffice of ScienceUniversity of Colorado BoulderAgencia Nacional de Investigación y DesarrolloLawrence Berkeley National LaboratoryYunnan UniversityJet Propulsion LaboratoryLeibniz-Institut für Astrophysik PotsdamChina National Textile and Apparel CouncilUniversity of Illinois at Urbana-ChampaignFermilabMax-Planck-Institut für AstronomieRheinische Friedrich-Wilhelms-Universität BonnMax-Planck-GesellschaftChinese Academy of SciencesDeutsche ForschungsgemeinschaftIntegrated Electronics Engineering Center, Binghamton UniversityUniversity of EdinburghSpace Telescope Science InstituteUniversity of SussexHeising-Simons FoundationCarnegie Institution for ScienceUniversity of NottinghamUniversity of ChicagoNational Energy Research Scientific Computing CenterUniversity of MichiganNational Science FoundationUK Research and InnovationUniversidad Nacional Autónoma de MéxicoScience and Technology Facilities CouncilEberhard Karls Universität TübingenAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Institution of WashingtonUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahHarvard UniversityOhio State UniversityFlatiron HealthSmithsonian InstitutionYale UniversityU.S. Department of EnergyUniversität HamburgNational Astronomical Observatories, Chinese Academy of SciencesCalifornia Institute of TechnologyUniversity College LondonNational Aeronautics and Space AdministrationFinanciadora de Estudos e ProjetosÉcole Polytechnique Fédérale de LausanneUniversity of PennsylvaniaNanjing UniversityUniversity of Toronto
KeywordsPhysicsAstrophysicsRedshiftAstronomyPhotometric redshiftPhotometry (optics)QuasarGalaxyStars

Abstract

fetched live from OpenAlex

Context . Computing reliable photometric redshifts (photo-z) for active galactic nuclei (AGN) is a challenging task, primarily due to the complex interplay between the unresolved relative emissions associated with the supermassive black hole and its host galaxy. Spectral energy distribution (SED) fitting methods, while effective for galaxies and AGN in pencil-beam surveys, face limitations in wide or all-sky surveys with fewer bands available, lacking the ability to accurately capture the AGN contribution to the SED, hindering reliable redshift estimation. This limitation is affecting the many tens of millions of AGN detected in existing datasets, such as those AGN clearly singled out and identified by SRG/eROSITA. Aims . Our goal is to enhance photometric redshift performance for AGN in all-sky surveys while simultaneously simplifying the approach by avoiding the need to merge multiple data sets. Instead, we employ readily available data products from the 10th Data Release of the Imaging Legacy Survey for the Dark Energy Spectroscopic Instrument, which covers >20 000 deg 2 of extragalactic sky with deep imaging and catalog-based photometry in the ɡriɀW1-W4 bands. We fully utilize the spatial flux distribution in the vicinity of each source to produce reliable photo-z. Methods . We introduce PICZL, a machine-learning algorithm leveraging an ensemble of convolutional neural networks. Utilizing a cross-channel approach, the algorithm integrates distinct SED features from images with those obtained from catalog-level data. Full probability distributions are achieved via the integration of Gaussian mixture models. Results . On a validation sample of 8098 AGN, PICZL achieves an accuracy σ NMAD of 4.5% with an outlier fraction η of 5.6%. These results significantly outperform previous attempts to compute accurate photo-z for AGN using machine learning. We highlight that the model’s performance depends on many variables, predominantly the depth of the data and associated photometric error. A thorough evaluation of these dependencies is presented in the paper. Conclusions . Our streamlined methodology maintains consistent performance across the entire survey area, when accounting for differing data quality. The same approach can be adopted for future deep photometric surveys such as LSST and Euclid, showcasing its potential for wide-scale realization. With this paper, we release updated photo-z (including errors) for the XMM-SERVS W-CDF-S, ELAIS-S1 and LSS fields.

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: Other design · Consensus signal: none
GenreCandidate signal: Methods · Consensus signal: none
Teacher disagreement score0.990
Threshold uncertainty score0.703

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 head0.221
Teacher spread0.214 · 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