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Record W3124433743 · doi:10.1093/mnras/stab085

Giant molecular cloud catalogues for PHANGS-ALMA: methods and initial results

2021· article· en· W3124433743 on OpenAlexafffund
Erik Rosolowsky, Annie Hughes, Adam K. Leroy, Jiayi Sun, Miguel Querejeta, Andreas Schruba, A. Usero, Cinthya N. Herrera, Daizhong Liu, J. Pety, Toshiki Saito, Ivana Bešlić, Frank Bigiel, Guillermo A. Blanc, Mélanie Chevance, Daniel A. Dale, Sinan Deger, Christopher M. Faesi, Simon C. O. Glover, Jonathan D. Henshaw, Ralf S. Klessen, J. M. Diederik Kruijssen, Kirsten L. Larson, Janice Lee, Sharon E. Meidt, Angus Mok, Eva Schinnerer, David A. Thilker, Thomas G. Williams

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsUniversity of Alberta
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesNational Institutes of Natural SciencesAstrophysics DivisionHorizon 2020 Framework ProgrammeNational Astronomical Observatory of JapanMinisterio de Ciencia e InnovaciónCentre National de la Recherche ScientifiqueCentre National d’Etudes SpatialesNatural Sciences and Engineering Research Council of CanadaNational Science CouncilDeutsche ForschungsgemeinschaftEuropean CommissionAgencia Estatal de InvestigaciónNational Radio Astronomy ObservatoryNational Science FoundationCompute CanadaMinisterio de Ciencia, Innovación y UniversidadesNational Aeronautics and Space AdministrationKorea Astronomy and Space Science Institute
KeywordsPhysicsAstrophysicsGalaxyMolecular cloudVirial theoremSpiral galaxyInitial mass functionAstronomyVirial massStar formationStars

Abstract

fetched live from OpenAlex

ABSTRACT We present improved methods for segmenting CO emission from galaxies into individual molecular clouds, providing an update to the cprops algorithms presented by Rosolowsky & Leroy. The new code enables both homogenization of the noise and spatial resolution among data, which allows for rigorous comparative analysis. The code also models the completeness of the data via false source injection and includes an updated segmentation approach to better deal with blended emission. These improved algorithms are implemented in a publicly available Python package, pycprops. We apply these methods to 10 of the nearest galaxies in the PHANGS-ALMA survey, cataloguing CO emission at a common 90 pc resolution and a matched noise level. We measure the properties of 4986 individual clouds identified in these targets. We investigate the scaling relations among cloud properties and the cloud mass distributions in each galaxy. The physical properties of clouds vary among galaxies, both as a function of galactocentric radius and as a function of dynamical environment. Overall, the clouds in our target galaxies are well-described by approximate energy equipartition, although clouds in stellar bars and galaxy centres show elevated line widths and virial parameters. The mass distribution of clouds in spiral arms has a typical mass scale that is 2.5× larger than interarm clouds and spiral arms clouds show slightly lower median virial parameters compared to interarm clouds (1.2 versus 1.4).

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)0.002
metaresearch head score (Gemma)0.006
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: Methods · Consensus signal: none
Teacher disagreement score0.036
Threshold uncertainty score0.071

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.006
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0050.003
Science and technology studies0.0010.000
Scholarly communication0.0020.001
Open science0.0020.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0070.005

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 head0.015
GPT teacher head0.282
Teacher spread0.267 · 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
GenreMethods

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

Citations150
Published2021
Admission routes2
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicAstrophysics and Star Formation StudiesFrench-language works237,207