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Record W4404353273 · doi:10.48550/arxiv.2411.01949

The first identification of Lyman $α$ Changing-look Quasars at high-redshift in DESI

2024· preprint· en· W4404353273 on OpenAlexfundno aff
Wei-Jian Guo, Zhiwei Pan, M. Siudek, J. Aguilar, S. P. Ahlen, Davide Bianchi, David H. Brooks, T. Claybaugh, Kyle Dawson, Axel de la Macorra, P. Doel, Kevin Fanning, J. E. Forero-Romero, E. Gaztañaga, Satya Gontcho A Gontcho, K. Honscheid, R. Kehoe, Theodore Kisner, Andrew Lambert, Martin Landriau, L. Le Guillou, Marc Manera, Aaron Meisner, John Moustakas, A. Muñoz-Gutiérrez, Adam D. Myers, Jundan Nie, N. Palanque‐Delabrouille, Claire Poppett, Francisco Prada, Mehdi Rezaie, Graziano Rossi, E. Sánchez, Michael Schubnelll, Hee‐Jong Seo, J. Silber, David Sprayberry, G. Tarlé, Benjamin A. Weaver, Zhimin Zhou, Hu Zou

Bibliographic record

VenuearXiv (Cornell University) · 2024
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsnot available
FundersHigh Energy PhysicsLawrence Berkeley National LaboratoryDivision of Astronomical SciencesScience and Technology Facilities CouncilUniversity of Colorado BoulderJet Propulsion LaboratoryInstituto de Astrofísica de CanariasOffice of ScienceMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikNarodowa Agencja Wymiany AkademickiejCommissariat à l'Énergie Atomique et aux Énergies AlternativesUniversidad Nacional Autónoma de MéxicoMinistério da Ciência, Tecnologia e InovaçãoSmithsonian InstitutionU.S. Department of EnergyNational Natural Science Foundation of ChinaChinese Academy of SciencesUniversity of OxfordYork UniversityLeibniz-GemeinschaftUniversity of Notre DameCarnegie Mellon UniversityUniversity of WashingtonJohns Hopkins UniversityNational Science FoundationOhio State UniversityCarnegie Institution of WashingtonMinisterio de Ciencia e InnovaciónEuropean CommissionCalifornia Institute of TechnologyCarnegie Institution for ScienceMinisterio de Ciencia, Innovación y UniversidadesGordon and Betty Moore FoundationNational Aeronautics and Space AdministrationNew Mexico State UniversityUniversity of PortsmouthAgencia Estatal de InvestigaciónYale UniversityVanderbilt University
KeywordsQuasarRedshiftAstrophysicsIdentification (biology)PhysicsAstronomyAlpha decayAlpha (finance)Lyman-alpha forestGalaxyIntergalactic mediumNuclear physicsMathematicsBiologyStatistics

Abstract

fetched live from OpenAlex

We present two cases of Ly$α$ changing-look (CL) quasars (J1306 and J1512) along with two additional candidates (J1511 and J1602), all discovered serendipitously at $z >2$ through the Dark Energy Spectroscopic Instrument (DESI) and the Sloan Digital Sky Survey (SDSS). It is the first time to capture CL events in Ly$α$ at high redshift, which is crucial for understanding underlying mechanisms driving the CL phenomenon and the evolution of high-redshift quasars and galaxies. The variability of all four sources is confirmed by the significant change of amplitude in the $r$ band ($|r_{\rm DESI}-r_{\rm SDSS}| >0.5 \ \rm mag$). We find that the accretion rate in the dim state for these CL objects corresponds to a relatively low value ($\mathscr{\dot M} \approx 2\times10^{-3}$), which suggests that the inner region of the accretion disk might be in transition between the Advection Dominated Accretion Flow ($\mathscr{\dot M}<10^{-3}\sim 10^{-2}$) and the canonical accretion disk (optically thick, geometrically thin). However, unlike in C {\sc iv} CL quasars in which broad Ly$α$ remained, the broad C {\sc iv} may still persist after a CL event occurs in Ly$α$, making the physical origin of the CL and ionization mechanism event more puzzling and interesting.

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 score0.004
Threshold uncertainty score0.008

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 studies0.0010.001
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.000

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 head0.033
GPT teacher head0.204
Teacher spread0.170 · 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

Citations0
Published2024
Admission routes1
Has abstractyes

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