MétaCan
Menu
Back to cohort
Record W3042552925 · doi:10.1093/pasj/psaa074

Subaru High-<i>z</i> Exploration of Low-Luminosity Quasars (SHELLQs). IX. Identification of two red quasars at <i>z</i> &amp;gt; 5.6

2020· article· en· W3042552925 on OpenAlexfundno aff
N. Kato, Yoshiki Matsuoka, Masafusa Onoue, Shuhei Koyama, Yoshiki Toba, Masayuki Akiyama, Seiji Fujimoto, Masatoshi Imanishi, K. Iwasawa, Takuma Izumi, Nobunari Kashikawa, Toshihiro Kawaguchi, Chien‐Hsiu Lee, Takeo Minezaki, Tohru Nagao, Akatoki Noboriguchi, Michael A. Strauss

Bibliographic record

VenuePublications of the Astronomical Society of Japan · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersPlanetary Science DivisionJapan Society for the Promotion of ScienceScience Mission DirectorateSmithsonian Astrophysical ObservatoryUniversity of California, Los AngelesMax-Planck-Institut für AstronomieToray Science FoundationHigh Energy Accelerator Research OrganizationNational Astronomical Observatory of JapanNational Central UniversityJapan Science and Technology AgencySmithsonian InstitutionMitsubishi FoundationMinistry of Education, Culture, Sports, Science and TechnologyQueen's UniversityCabinet Office, Government of JapanSpace Telescope Science InstitutePrinceton UniversityJohns Hopkins UniversityJet Propulsion LaboratoryQueen's University BelfastDurham UniversityUniversity of MarylandNational Aeronautics and Space AdministrationEötvös Loránd TudományegyetemAcademia SinicaCalifornia Institute of TechnologyNational Science Foundation
KeywordsQuasarPhysicsAstrophysicsIdentification (biology)LuminosityAstronomyGalaxy

Abstract

fetched live from OpenAlex

Abstract We present the first discovery of dust-reddened quasars (red quasars) in the high-z universe (z &amp;gt; 5.6). This is a result from the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) project, which is based on the sensitive multi-band optical imaging data produced by the Hyper Suprime-Cam (HSC) Subaru Strategic Program survey. We identified four red quasar candidates from the 93 spectroscopically confirmed high-z quasars in the SHELLQs sample, based on detections in the Wide-field Infrared Survey Explorer (WISE) data at 3.4 and 4.6 μm (rest-frame ∼5000–6500 Å). The amount of dust reddening was estimated with spectral energy distribution (SED) fits over optical and mid-infrared wavelengths. Two of the four candidates were found to be red quasars with dust reddening of E(B − V) &amp;gt; 0.1. The remaining SHELLQs quasars without individual WISE detections are significantly fainter in the WISE bands and bluer than the red quasars, although we did detect them in the W1 band in a stacked image. We also conducted the same SED fits for high-z optically-luminous quasars, but no red quasar was found. This demonstrates the power of Subaru HSC to discover high-z red quasars, which are fainter than the limiting magnitudes of past surveys in the rest-frame ultraviolet, due to dust extinction.

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 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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.880

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0000.001
Science and technology studies0.0000.001
Scholarly communication0.0000.001
Open science0.0010.000
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 head0.020
GPT teacher head0.230
Teacher spread0.210 · 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 teacher head, 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

Citations19
Published2020
Admission routes1
Has abstractyes

Explore more

Same venuePublications of the Astronomical Society of JapanSame topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207