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Record W2950509913 · doi:10.1088/0004-637x/753/1/33

A POPULATION OF DUST-RICH QUASARS AT<i>z</i>∼ 1.5

2012· article· fa· W2950509913 on OpenAlexafffund
Y. Sophia Dai, J. Bergeron, M. Elvis, A. Omont, Jia-Sheng Huang, Jamie Bock, Asantha Cooray, G. G. Fazio, E. Hatziminaoglou, G. Magdis, S. Oliver, Mathew Page, I. Pérez‐Fournon, D. Rigopoulou, Isaac G. Roseboom, D. Scott, M. Symeonidis, Markos Trichas, J. D. Vieira, Christopher N. A. Willmer, M. Zemcov

Bibliographic record

VenueThe Astrophysical Journal · 2012
Typearticle
Languagefa
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of British Columbia
FundersNational Astronomical Observatories, Chinese Academy of SciencesScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryCentre National de la Recherche ScientifiqueUniversità degli Studi di PadovaJet Propulsion LaboratoryCentre National d’Etudes SpatialesCardiff UniversityImperial College LondonUniversity of LethbridgeCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationUK Space AgencyUniversity of SussexSmithsonian Institution
KeywordsQuasarAstrophysicsPhysicsRedshiftGalaxyInfraredPopulationAstronomyLuminous infrared galaxy

Abstract

fetched live from OpenAlex

We report Herschel SPIRE (250, 350, and 500 μm) detections of 32 quasars with redshifts 0.5 ⩽ z < 3.6 from the Herschel Multi-tiered Extragalactic Survey (HerMES). These sources are from a MIPS 24 μm flux-limited sample of 326 quasars in the Lockman Hole Field. The extensive multi-wavelength data available in the field permit construction of the rest-frame spectral energy distributions (SEDs) from ultraviolet to the mid-infrared for all sources, and to the far-infrared (FIR) for the 32 objects. Most quasars with Herschel FIR detections show dust temperatures in the range of 25–60 K, with a mean of 34 K. The FIR luminosities range from 10 11.3 to 10 13.5 L ☉ , qualifying most of their hosts as ultra- or hyper-luminous infrared galaxies. These FIR-detected quasars may represent a dust-rich population, but with lower redshifts and fainter luminosities than quasars observed at ∼1 mm. However, their FIR properties cannot be predicted from shorter wavelengths (0.3–20 μm, rest frame), and the bolometric luminosities derived using the 5100 Å index may be underestimated for these FIR-detected quasars. Regardless of redshift, we observed a decline in the relative strength of FIR luminosities for quasars with higher near-infrared luminosities.

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 score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.011
GPT teacher head0.226
Teacher spread0.215 · 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

Citations37
Published2012
Admission routes2
Has abstractyes

Explore more

Same venueThe Astrophysical Journal→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→