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Record W4411946253 · doi:10.1051/0004-6361/202554355

Narrow absorption lines from intervening material in supernovae

2025· article· en· W4411946253 on OpenAlexfundno aff
S. González–Gaitán, E. Tomás Müller-Bravo, Poul Anderson, L. Galbany, M. Sullivan, João Rino-Silvestre, Mariona Caixach, A. Morales-Garoffolo, Sabyasachi Goswami, S. Mattila

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryLos Alamos National LaboratoryArgonne National LaboratoryAgencia Estatal de InvestigaciónCentro de Investigaciones Energéticas, Medioambientales y TecnológicasFundação para a Ciência e a TecnologiaLeibniz-GemeinschaftScience Mission DirectorateUniversity of Colorado BoulderUniversity of Illinois at Urbana-ChampaignFermilabMax-Planck-Institut für AstronomieLeibniz-Institut für Astrophysik PotsdamChina National Textile and Apparel CouncilEötvös Loránd TudományegyetemEuropean Regional Development FundCentre National de la Recherche ScientifiqueYale UniversityU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoScience and Technology Facilities CouncilMinistério da Ciência, Tecnologia e InovaçãoUniversity of TorontoGeneralitat de CatalunyaDeutsche ForschungsgemeinschaftDurham UniversityIntegrated Electronics Engineering Center, Binghamton UniversityQueen's UniversityUniversity of EdinburghNational Central UniversityInstitut de Física d'Altes EnergiesSpace Telescope Science InstituteUniversity of SussexUniversity of NottinghamJohns Hopkins UniversityMinisterio de Ciencia e InnovaciónEuropean CommissionNational Aeronautics and Space AdministrationUniversity College LondonUniversity of CambridgeUniversidad Nacional Autónoma de MéxicoSmithsonian Astrophysical ObservatoryEuropean Space AgencyAlfred P. Sloan FoundationUniversity of ChicagoHarvard UniversityOhio State UniversityNational Science FoundationUniversity of MichiganPlanetary Science DivisionCarnegie Institution of WashingtonFlatiron HealthSmithsonian InstitutionNational Astronomical Observatories, Chinese Academy of SciencesCalifornia Institute of TechnologyFinanciadora de Estudos e ProjetosÉcole Polytechnique Fédérale de LausanneUniversity of PennsylvaniaQueen's University BelfastMinisterio de Ciencia, Innovación y UniversidadesGordon and Betty Moore FoundationNanjing UniversityNew Mexico State UniversityUniversity of PortsmouthLawrence Berkeley National LaboratoryYunnan University
KeywordsPhysicsAstrophysicsSupernovaGalaxyAstronomyAbsorption (acoustics)Optics

Abstract

fetched live from OpenAlex

The interstellar medium (ISM) has a number of tracers such as the NaI Dλλ 5890, 5896 absorption lines that are evident in the spectra of galaxies but also in those of individual astrophysical sources such as stars, novae, or quasars. Here, we investigate narrow absorption features in the spectra of nearby supernovae (SNe) and compare them to local (<0.5 kpc) and global host galaxy properties. With a large and heterogeneous sample of spectra, we are able to recover the known relations of ISM with galaxy properties: larger columns of ISM gas are found in environments that are more massive, more actively star-forming, younger, and viewed from a more inclined angle. Most trends are stronger for local properties than global properties, and we find that the ISM column density decreases exponentially with the offset from the host galaxy centre, as expected for a gas distribution following an exponential radial profile. We also confirm trends for the velocity of galactic outflows increasing with radius. The current study demonstrates the capability of individual light sources to serve as ubiquitous tracers of ISM properties across various environments and galaxies.

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 score0.001
Threshold uncertainty score0.004

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 communication0.0010.000
Open science0.0000.000
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 head0.008
GPT teacher head0.221
Teacher spread0.214 · 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
Published2025
Admission routes1
Has abstractyes

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