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Record W3200356422 · doi:10.1093/mnras/stab2742

Ionizing radiation from AGNs at <i>z</i> &amp;gt; 3.3 with the Subaru Hyper Suprime-Cam Survey and the CFHT Large Area U-band Deep Survey (CLAUDS)

2021· article· en· W3200356422 on OpenAlexafffund
Ikuru Iwata, Marcin Sawicki, Akio Inoue, Masayuki Akiyama, Genoveva Micheva, Toshihiro Kawaguchi, Nobunari Kashikawa, Stephen Gwyn, S. Arnouts, Jean Coupon, G. Desprez

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsHerzberg Institute of AstrophysicsSaint Mary's University
FundersPlanetary Science DivisionNational Astronomical Observatories, Chinese Academy of SciencesJapan Society for the Promotion of ScienceNational Research Council CanadaScience Mission DirectorateEötvös Loránd TudományegyetemNational Astronomical Observatory of JapanNational Central UniversityCentre National de la Recherche ScientifiqueToray Science FoundationHigh Energy Accelerator Research OrganizationUniversity of TokyoMax-Planck-GesellschaftCabinet Office, Government of JapanUniversity of MarylandChinese Academy of SciencesJapan Science and Technology AgencyU.S. Department of EnergySmithsonian InstitutionCanadian Foundation for AIDS ResearchJapan Science and Technology CorporationQueen's University BelfastMax-Planck-Institut für AstronomieUniversity of EdinburghSpace Telescope Science InstituteSmithsonian Astrophysical ObservatoryHuntington Society of CanadaCalifornia Earthquake AuthorityQueen's UniversityMinistry of Education, Culture, Sports, Science and TechnologyAlfred P. Sloan FoundationPrinceton UniversityJohns Hopkins UniversityNatural Sciences and Engineering Research Council of CanadaDurham UniversityFoundation for Ichthyosis and Related Skin TypesMinistry of FinanceHigher Education Funding Council for EnglandNational Aeronautics and Space AdministrationUniversity of Hawai'iAcademia SinicaCompute CanadaNational Science Foundation
KeywordsPhysicsAstrophysicsRedshiftPhotometry (optics)Flux (metallurgy)Ionizing radiationAstronomyActive galactic nucleusGalaxyStarsIrradiationNuclear physics

Abstract

fetched live from OpenAlex

ABSTRACT We use deep and wide imaging data from the CFHT Large Area U-band Deep Survey (CLAUDS) and the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) to constrain the ionizing radiation (Lyman Continuum, LyC) escape fraction from active galactic nuclei (AGNs) at z ∼ 3–4. For 94 AGNs with spectroscopic redshifts at 3.3 < z < 4.0, we use their U/i-band flux ratios to estimate LyC transmission of individual AGNs. The distribution of their LyC transmission shows values lower than the range of LyC transmission values for IGM of the same redshift range, which suggests that LyC escape fraction of AGNs at z > 3.3 is considerably lower than unity in most cases. We do not find any trend in LyC transmission values depending on their UV luminosities. Based on the photometry of stacked images we find the average flux ratio of LyC and non-ionizing UV photons escaping from the objects (fLyC/fUV)out = 0.182 ± 0.043 for AGNs at 3.3 < z < 3.6, which corresponds to LyC escape fraction fesc = 0.303 ± 0.072 if we assume a fiducial intrinsic SED of AGN. Based on the estimated LyC escape fraction and the UV luminosity function (UVLF) of AGNs, we argue that UV-selected AGNs’ contribution to the LyC emissivity at the epoch is minor, although the size of their contribution largely depends on the shape of the UVLF.

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)0.000
metaresearch head score (Gemma)0.000
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: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.021
Threshold uncertainty score0.041

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.009
GPT teacher head0.188
Teacher spread0.178 · 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

Citations14
Published2021
Admission routes2
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→