MétaCan
Menu
← Back to cohort
Record W4383605198 · doi:10.48550/arxiv.2307.03182

Long-term follow-up observations of extreme coronal line emitting galaxies

2023· preprint· en· W4383605198 on OpenAlexfundno aff
P. Clark, Or Graur, J. Aguilar, S. P. Ahlen, J. P. Anderson, E. Berger, Thomas G. Brink, David H. Brooks, T. W. Chen, T. Claybaugh, Axel de la Macorra, P. Doel, A. V. Filippenko, Sebastián Gómez, M. Gromadzki, K. Honscheid, C. Inserra, Theodore Kisner, Martin Landriau, L. Makrygianni, Marc Manera, Aaron Meisner, Ramon Miquel, John Moustakas, T. E. Müller-Bravo, Matt Nicholl, Jundan Nie, F. Onori, A. Palmese, Claire Poppett, T. Reynolds, Mehdi Rezaie, Graziano Rossi, E. Sánchez, M. Schubnell, G. Tarlé, Benjamin Alan Weaver, T. Wevers, D. R. Young, WeiKang Zheng, Zhimin Zhou

Bibliographic record

VenuearXiv (Cornell University) · 2023
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersPlanetary Science DivisionDivision of Astronomical SciencesInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilAgencia Estatal de InvestigaciónScience Mission DirectorateUniversity of California ObservatoriesSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryOffice of ScienceMax-Planck-Institut für AstronomieEötvös Loránd TudományegyetemStockholms UniversitetDeutsches Elektronen-SynchrotronCommissariat à l'Énergie Atomique et aux Énergies AlternativesQueen's UniversityGordon and Betty Moore FoundationQueen's University BelfastSpace Telescope Science InstituteLos Alamos National LaboratoryAlfred P. Sloan FoundationUniversity of WashingtonJohns Hopkins UniversityEuropean CommissionMinisterio de Ciencia e InnovaciónUniversity of UtahUniversity of WarwickDurham UniversityNorthwestern UniversityNational Science FoundationAgencia Nacional de Investigación y DesarrolloTrinity College DublinSmithsonian InstitutionU.S. Department of EnergyCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationNational Central UniversityNuclear Safety and Security Commission
KeywordsAstrophysicsPhysicsLine (geometry)SkyGalaxyAstronomyActive galactic nucleusLight curveSpectral lineCoronal planeEmission spectrum

Abstract

fetched live from OpenAlex

We present new spectroscopic and photometric follow-up observations of the known sample of extreme coronal line emitting galaxies (ECLEs) identified in the Sloan Digital Sky Survey (SDSS). With these new data, observations of the ECLE sample now span a period of two decades following their initial SDSS detections. We confirm the nonrecurrence of the iron coronal line signatures in five of the seven objects, further supporting their identification as the transient light echoes of tidal disruption events (TDEs). Photometric observations of these objects in optical bands show little overall evolution. In contrast, mid-infrared (MIR) observations show ongoing long-term declines. The remaining two objects had been classified as active galactic nuclei (AGN) with unusually strong coronal lines rather than being TDE related, given the persistence of the coronal lines in earlier follow-up spectra. We confirm this classification, with our spectra continuing to show the presence of strong, unchanged coronal-line features and AGN-like MIR colours and behaviour. We have constructed spectral templates of both subtypes of ECLE to aid in distinguishing the likely origin of newly discovered ECLEs. We highlight the need for higher cadence, and more rapid, follow-up observations of such objects to better constrain their properties and evolution. We also discuss the relationships between ECLEs, TDEs, and other identified transients having significant MIR variability.

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)0.001
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 score0.003
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
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 science0.0000.001
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 head0.167
GPT teacher head0.216
Teacher spread0.049 · 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

Citations2
Published2023
Admission routes1
Has abstractyes

Explore more

Same venuearXiv (Cornell University)→Same topicStellar, planetary, and galactic studies→French-language works237,207→