MétaCan
Menu
Back to cohort
Record W4414371049 · doi:10.1093/mnras/staf1560

A deep search for diffuse interstellar band 4430 Å in the circumgalactic medium

2025· article· en· W4414371049 on OpenAlexfundno aff
Chih-Yuan Chang, Ting-Wen Lan

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicSuperconducting and THz Device Technology
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratoryUniversity of Colorado BoulderInstituto de Astrofísica de CanariasOffice of ScienceMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikUniversity of OxfordMinistry of Education, IndiaYork UniversityMinistry of Science and TechnologyMinistério da Ciência, Tecnologia e InovaçãoMinistry of EducationLeibniz-GemeinschaftUniversity of Notre DameCarnegie Mellon UniversityUniversidad Nacional Autónoma de MéxicoAlfred P. Sloan FoundationUniversity of WashingtonJohns Hopkins UniversityCarnegie Institution of WashingtonUniversity of UtahNational Taiwan UniversityNational Science and Technology CouncilU.S. Department of EnergySmithsonian InstitutionNew Mexico State UniversityUniversity of PortsmouthVanderbilt UniversityYale UniversityOhio State University
KeywordsMilky WaySpectral lineAbsorption (acoustics)Interstellar mediumSkyAbsorption spectroscopyLine (geometry)

Abstract

fetched live from OpenAlex

ABSTRACT We investigate the absorption signals of one of the strongest diffuse interstellar bands, DIB$\lambda 4430$, in the circumgalactic medium (CGM) traced by Mg ii absorption lines. To this end, we make use of approximately 60 000 Mg ii absorption line spectra within $0.4 < z < 1.0$ compiled from the Sloan Digital Sky Surveys and obtain composite spectra with uncertainties for absorption line measurements being a few mÅ. By using Mg ii absorption strength and dust reddening relation from the literature, we measure the DIB$\lambda 4430$ absorption strength as a function of E(B – V) in the CGM, and compare the Milky Way DIB$\lambda 4430$ –E(B – V) relation extrapolated down to the CGM E(B – V) region. Our results show no detectable signals of DIB$\lambda 4430$ across the entire E(B – V) range in the CGM traced by Mg ii absorption lines. This lack of detection of DIB$\lambda 4430$ in the CGM is inconsistent with the Milky Way signals by $\sim 5 \, \sigma$, indicating that the factors associated with different environments affect the abundance of the DIB$\lambda 4430$ carrier.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.716
Threshold uncertainty score0.396

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
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 head0.012
GPT teacher head0.244
Teacher spread0.232 · 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

Citations1
Published2025
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicSuperconducting and THz Device TechnologyFrench-language works237,207