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Record W4400717818 · doi:10.1051/0004-6361/202450886

CIRCLEZ : Reliable photometric redshifts for active galactic nuclei computed solely using photometry from Legacy Survey Imaging for DESI

2024· preprint· en· W4400717818 on OpenAlexfundno aff
M. Salvato, W. Roster, R. Shirley, Johannes Büchner, J. Wolf, C. P. Kohl, H. Starck, T. Dwelly, Johan Comparat, A. Malyali, Sven Krippendorf, A. Zenteno, Dustin Lang, D. Schlegel, Rongpu Zhou, A. Dey, F. Valdes, A. Myers, R. J. Assef, Cláudio Ricci, Matthew J. Temple, A. Merloni, Anton M. Koekemoer, Scott F. Anderson, X. Liu, K. Nandra

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typepreprint
Languageen
FieldEngineering
TopicCCD and CMOS Imaging Sensors
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryArgonne National LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityHigh Energy PhysicsDivision of Astronomical SciencesRussian Academy of SciencesLeibniz-GemeinschaftEberhard Karls Universität TübingenScience and Technology Facilities CouncilUniversity of Colorado BoulderOffice of ScienceFermilabRheinische Friedrich-Wilhelms-Universität BonnMax-Planck-Institut für AstronomieAgencia Nacional de Investigación y DesarrolloLawrence Berkeley National LaboratoryYunnan UniversityJet Propulsion LaboratoryLeibniz-Institut für Astrophysik PotsdamChina National Textile and Apparel CouncilUniversity of Illinois at Urbana-ChampaignMax-Planck-GesellschaftChinese Academy of SciencesDeutsche ForschungsgemeinschaftSpace Telescope Science InstituteUniversity of SussexNational Aeronautics and Space AdministrationUniversity College LondonUniversity of ChicagoNational Energy Research Scientific Computing CenterHeising-Simons FoundationCarnegie Institution for ScienceUniversity of NottinghamUniversidad Nacional Autónoma de MéxicoAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Institution of WashingtonUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahHarvard UniversityOhio State UniversitySmithsonian Astrophysical ObservatoryFlatiron HealthSmithsonian InstitutionYale UniversityU.S. Department of EnergyUniversität HamburgNational Astronomical Observatories, Chinese Academy of SciencesCalifornia Institute of TechnologyFinanciadora de Estudos e ProjetosÉcole Polytechnique Fédérale de LausanneUniversity of PennsylvaniaNanjing UniversityUniversity of TorontoNational Science Foundation
KeywordsPhotometry (optics)RedshiftPhotometric redshiftAstronomyAstrophysicsPhysicsGalaxyStars

Abstract

fetched live from OpenAlex

Context. Photometric redshifts for galaxies hosting an accreting supermassive black hole in their center, known as active galactic nuclei (AGNs), are notoriously challenging. At present, they are most optimally computed via spectral energy distribution (SED) fittings, assuming that deep photometry for many wavelengths is available. However, for AGNs detected from all-sky surveys, the photometry is limited and provided by a range of instruments and studies. This makes the task of homogenizing the data challenging, presenting a dramatic drawback for the millions of AGNs that wide surveys such as SRG/eROSITA are poised to detect. Aims. This work aims to compute reliable photometric redshifts for X-ray-detected AGNs using only one dataset that covers a large area: the tenth data release of the Imaging Legacy Survey (LS10) for DESI. LS10 provides deep grizW1-W4 forced photometry within various apertures over the footprint of the eROSITA-DE survey, which avoids issues related to the cross-calibration of surveys. Methods. We present the results from C IRCLE Z, a machine-learning algorithm based on a fully connected neural network. C IRCLE Z is built on a training sample of 14 000 X-ray-detected AGNs and utilizes multi-aperture photometry, mapping the light distribution of the sources. Results. The accuracy ( σ NMAD ) and the fraction of outliers ( η ) reached in a test sample of 2913 AGNs are equal to 0.067 and 11.6%, respectively. The results are comparable to (or even better than) what was previously obtained for the same field, but with much less effort in this instance. We further tested the stability of the results by computing the photometric redshifts for the sources detected in CSC2 and Chandra -COSMOS Legacy, reaching a comparable accuracy as in eFEDS when limiting the magnitude of the counterparts to the depth of LS10. Conclusions. The method can be applied to fainter samples of AGNs using deeper optical data from future surveys (for example, LSST, Euclid ), granting LS10-like information on the light distribution beyond the morphological type. Along with this paper, we have released an updated version of the photometric redshifts (including errors and probability distribution functions) for eROSITA/eFEDS.

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)0.007
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Methods · Consensus signal: none
Teacher disagreement score0.027
Threshold uncertainty score0.054

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.007
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0030.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0020.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0030.003

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 head0.246
Teacher spread0.225 · 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 designSimulation or modeling
Domainnot available
GenreMethods

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

Citations15
Published2024
Admission routes1
Has abstractyes

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