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Record W4221155515 · doi:10.3847/1538-4357/ac58f9

Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 0346–52

2022· article· en· W4221155515 on OpenAlexaff
Katrina C. Litke, Daniel P. Marrone, Manuel Aravena, M. Béthermin, S. C. Chapman, Chenxing Dong, Christopher C. Hayward, Ryley Hill, Sreevani Jarugula, Matthew A. Malkan, Desika Narayanan, C. Reuter, Justin Spilker, Nikolaus Sulzenauer, J. D. Vieira, A. Weiß

Bibliographic record

VenueThe Astrophysical Journal · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of British ColumbiaDalhousie University
FundersNational Astronomical Observatory of JapanInternational Max Planck Research School for Advanced Methods in Process and Systems EngineeringMax-Planck-GesellschaftNational Institutes of Natural SciencesInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologySpace Telescope Science InstituteAlfred P. Sloan FoundationAgencia Nacional de Investigación y DesarrolloKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationNational Radio Astronomy ObservatoryNational Science Foundation
KeywordsPhysicsAstrophysicsGalaxyInterstellar mediumMetallicityStar formationAstronomyPhotoionizationIonization

Abstract

fetched live from OpenAlex

Abstract With Σ SFR ∼ 4200 M ⊙ yr −1 kpc −2 , SPT 0346–52 ( z = 5.7) is the most intensely star-forming galaxy discovered by the South Pole Telescope. In this paper, we expand on previous spatially resolved studies, using ALMA observations of dust continuum, [N ii ] 205 μ m, [C ii ] 158 μ m, [O i ] 146 μ m, and undetected [N ii ] 122 μ m and [O i ] 63 μ m emission to study the multiphase interstellar medium (ISM) in SPT 0346–52. We use pixelated, visibility-based lens modeling to reconstruct the source-plane emission. We also model the source-plane emission using the photoionization code cloudy and find a supersolar metallicity system. We calculate T dust = 48.3 K and λ peak = 80 μ m and see line deficits in all five lines. The ionized gas is less dense than comparable galaxies, with n e < 32 cm −3 , while ∼20% of the [C ii ] 158 μ m emission originates from the ionized phase of the ISM. We also calculate the masses of several phases of the ISM. We find that molecular gas dominates the mass of the ISM in SPT 0346–52, with the molecular gas mass ∼4× higher than the neutral atomic gas mass and ∼100× higher than the ionized gas mass.

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 score0.013
Threshold uncertainty score0.025

Distilled classifier scores by category (both heads)

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 communication0.0010.000
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 head0.013
GPT teacher head0.240
Teacher spread0.228 · 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

Citations13
Published2022
Admission routes1
Has abstractyes

Explore more

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