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Record W2991000715 · doi:10.1093/mnras/stz3264

Are galactic star formation and quenching governed by local, global, or environmental phenomena?

2019· article· en· W2991000715 on OpenAlexafffund
Asa F. L. Bluck, R. Maiolino, S. F. Sánchez, Sara L. Ellison, Mallory Thorp, Joanna M. Piotrowska, Hossen Teimoorinia, Kevin Bundy

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsHerzberg Institute of AstrophysicsUniversity of Victoria
FundersLawrence Berkeley National LaboratoryH2020 European Research CouncilSmithsonian Astrophysical ObservatoryOffice of ScienceMax-Planck-Institut für AstronomieFondation MeracMax-Planck-GesellschaftMinistério da Ciência, Tecnologia e InovaçãoChinese Academy of SciencesNatural Sciences and Engineering Research Council of CanadaYork UniversityHigher Education Funding Council for EnglandNew Mexico State UniversityUniversity of PortsmouthUniversity of OxfordPennsylvania State UniversityUniversity of VirginiaScience and Technology Facilities CouncilUniversity of Colorado BoulderUniversität BaselFermilabNational Science FoundationCase Western Reserve UniversityCarnegie Mellon UniversityUniversity of PittsburghLeibniz-GemeinschaftUniversity of Notre DameUniversity of ArizonaLos Alamos National LaboratoryUniversity of WashingtonPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Institution of WashingtonUniversity of UtahUniversity of TokyoOhio State UniversityNew York UniversityConsejo Nacional de Ciencia y TecnologíaVanderbilt UniversityDrexel UniversityU.S. Naval ObservatoryU.S. Department of EnergySmithsonian InstitutionNational Aeronautics and Space AdministrationYale University
KeywordsPhysicsAstrophysicsStar formationQuenching (fluorescence)Star (game theory)AstronomyGalaxyQuantum mechanics

Abstract

fetched live from OpenAlex

ABSTRACT We present an analysis of star formation and quenching in the SDSS-IV MaNGA-DR15, utilizing over 5 million spaxels from ∼3500 local galaxies. We estimate star formation rate surface densities (ΣSFR) via dust corrected H α flux where possible, and via an empirical relationship between specific star formation rate (sSFR) and the strength of the 4000 Å break (D4000) in all other cases. We train a multilayered artificial neural network (ANN) and a random forest (RF) to classify spaxels into ‘star-forming’ and ‘quenched’ categories given various individual (and groups of) parameters. We find that global parameters (pertaining to the galaxy as a whole) perform collectively the best at predicting when spaxels will be quenched, and are substantially superior to local/spatially resolved and environmental parameters. Central velocity dispersion is the best single parameter for predicting quenching in central galaxies. We interpret this observational fact as a probable consequence of the total integrated energy from active galactic neucleus (AGN) feedback being traced by the mass of the black hole, which is well known to correlate strongly with central velocity dispersion. Additionally, we train both an ANN and RF to estimate ΣSFR values directly via regression in star-forming regions. Local/spatially resolved parameters are collectively the most predictive at estimating ΣSFR in these analyses, with stellar mass surface density at the spaxel location (Σ*) being by far the best single parameter. Thus, quenching is fundamentally a global process but star formation is governed locally by processes within each spaxel.

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: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.195
Threshold uncertainty score0.680

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 communication0.0000.001
Open science0.0000.000
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 head0.005
GPT teacher head0.180
Teacher spread0.176 · 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

Citations135
Published2019
Admission routes2
Has abstractyes

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