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Record W4321455632 · doi:10.1017/pasa.2023.7

AllBRICQS: The All-sky BRIght, Complete Quasar Survey

2023· article· en· W4321455632 on OpenAlexfundno aff
Christopher A. Onken, Christian Wolf, Wei Jeat Hon, Samuel Lai, P. Tisserand, R. L. Webster

Bibliographic record

VenuePublications of the Astronomical Society of Australia · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersIntegrated Electronics Engineering Center, Binghamton UniversityNational Cancer InstituteAustralian Astronomical Optics-MacquarieScience Mission DirectorateSmithsonian Astrophysical ObservatoryUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstronomieInstitut de Física d'Altes EnergiesEötvös Loránd TudományegyetemCurtin University of TechnologyGordon and Betty Moore FoundationSwinburne University of TechnologyQueen's University BelfastAustralian GovernmentAustralian Research CouncilSpace Telescope Science InstituteUniversity of PortsmouthLos Alamos National LaboratoryAustralian National Data ServiceJohns Hopkins UniversityNational Computational InfrastructureNational Aeronautics and Space AdministrationUniversity College LondonSLAC National Accelerator LaboratoryQueen's UniversityOhio State UniversityAustralian National UniversityAstronomy Australia LimitedDurham UniversitySmithsonian InstitutionCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorLawrence Berkeley National LaboratoryUniversity of PennsylvaniaArgonne National LaboratoryPlanetary Science DivisionMonash UniversityNational Central UniversityUniversity of SussexFermilabNational Science Foundation
KeywordsQuasarPhysicsAstrophysicsSkyRedshiftAstronomyOVV quasarGalaxy

Abstract

fetched live from OpenAlex

Abstract We describe the first results from the All-sky BRIght, Complete Quasar Survey (AllBRICQS), which aims to discover the last remaining optically bright quasars. We present 156 spectroscopically confirmed quasars (140 newly identified) having $|b|>10^{\circ}$ . 152 of the quasars haveGaiaDR3 magnitudes brighter than $B_{P}=16.5$ or $R_{P}=16$ mag, while four are slightly fainter. The quasars span a redshift range of $z=0.07-3.93$ . In particular, we highlight the properties of J0529-4351 at $z=3.93$ , which, if unlensed, is one of the most intrinsically luminous quasars in the Universe. The AllBRICQS sources have been selected by combining data from theGaiaandWISEall-sky satellite missions, and we successfully identify quasars not flagged as candidates byGaiaData Release 3. We expect the completeness to be $\approx$ 96% within our magnitude and latitude limits, while the preliminary results indicate a selection purity of $\approx$ 96%. The optical spectroscopy used for source classification will also enable detailed quasar characterisation, including black hole mass measurements and identification of foreground absorption systems. The AllBRICQS sources will greatly enhance the number of quasars available for high-signal-to-noise follow-up with present and future facilities.

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)0.001
metaresearch head score (Gemma)0.001
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 score0.046
Threshold uncertainty score0.091

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0050.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0080.003

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 head0.062
GPT teacher head0.282
Teacher spread0.220 · 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
Published2023
Admission routes1
Has abstractyes

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