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Record W2799187493 · doi:10.3847/1538-4357/aabd82

A First Look at BISTRO Observations of the ρ Oph-A core

2018· article· en· W2799187493 on OpenAlexaff
Jungmi Kwon, Yasuo Doi, Motohide Tamura, M. Matsumura, Kate Pattle, David Berry, Sarah Sadavoy, Brenda C. Matthews, D. Ward–Thompson, Tetsuo Hasegawa, Ray S. Furuya, Andy Pon, James Di Francesco, D. Arzoumanian, Saeko S. Hayashi, Koji S. Kawabata, Takashi Onaka, Minho Choi, Miju Kang, Thiem Hoang, Chang Won Lee, Sang-Sung Lee, Hongli Liu, Tie Liu, Shu‐ichiro Inutsuka, Chakali Eswaraiah, Pierre Bastien, Woojin Kwon, S. Lai, Keping Qiu, Simon Coudé, Erica Franzmann, Per Friberg, Sarah Graves, J. S. Greaves, Martin Houde, Doug Johnstone, J. M. Kirk, Patrick M. Koch, Di Li, Harriet Parsons, Ramprasad Rao, Mark G. Rawlings, Hiroko Shinnaga, S. Van Loo, Yusuke Aso, Do‐Young Byun, Huei-Ru Vivien Chen, Mike Chen, Wen-Ping Chen, Tao-Chung Ching, Jungyeon Cho, A. Chrysostomou, Eun Jung Chung, E. Drabek-Maunder, S. P. S. Eyres, Jason Fiege, Rachel Friesen, G. A. Fuller, T. M. Gledhill, M. J. Griffin, Qilao Gu, J. Hatchell, W. S. Holland, Tsuyoshi Inoue, Kazunari Iwasaki, Il-Gyo Jeong, Ji‐hyun Kang, Sung-Ju Kang, F. Kemper, Gwanjeong Kim, Jongsoo Kim, Kee‐Tae Kim, Kyoung Hee Kim, Mi-Ryang Kim, Shinyoung Kim, Kevin Lacaille, Jeong‐Eun Lee, Hua-bai Li, Junhao Liu, Sheng‐Yuan Liu, A-Ran Lyo, Steve Mairs, G. H. Moriarty‐Schieven, Fumitaka Nakamura, Hiroyuki Nakanishi, Nagayoshi Ohashi, N. Peretto, Tae‐Soo Pyo, Lei Qian, Brendan Retter, John Richer, A. J. Rigby, Jean-Franois Robitaille, G. Savini, Anna M. M. Scaife, Archana Soam, Ya‐Wen Tang, Kohji Tomisaka, Hongchi Wang, Jia-Wei Wang, A. P. Whitworth, Hsi-Wei Yen, Hyunju Yoo, Jinghua Yuan, Chuan-Peng Zhang, Guoyin Zhang, Jianjun Zhou, P. André, C. D. Dowell, S. A. E. G. Falle, Yusuke Tsukamoto, Takao Nakagawa, Yoshihiro Kanamori, Akimasa Kataoka, Masato I. N. Kobayashi, Tetsuya Nagata, Hiro Saito, Masumichi Seta, Tetsuya Zenko

Bibliographic record

VenueThe Astrophysical Journal · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsMcMaster UniversityDalhousie UniversityUniversity of ManitobaWestern UniversityUniversité de MontréalCentre for Research in Astrophysics of QuébecUniversity of VictoriaHerzberg Institute of Astrophysics
FundersNational Institutes of Natural SciencesJapan Society for the Promotion of ScienceEast Asian Core Observatories AssociationNational Astronomical Observatory of JapanMinistry of Education, Culture, Sports, Science and TechnologyMinistry of Science and Technology, TaiwanNational Research Foundation of KoreaKorea Astronomy and Space Science InstituteNederlandse Organisatie voor Wetenschappelijk OnderzoekAcademia SinicaChinese Academy of SciencesMinistry of Science, ICT and Future PlanningScience and Technology Facilities CouncilNational Research Foundation
KeywordsPhysicsPolarization (electrochemistry)SkyPolarimetryAstrophysicsMagnetic fieldPolarimeterFaraday effectInfraredAstronomyOpticsScattering

Abstract

fetched live from OpenAlex

Abstract We present 850 μ m imaging polarimetry data of the ρ Oph-A core taken with the Submillimeter Common-User Bolometer Array-2 (SCUBA-2) and its polarimeter (POL-2) as part of our ongoing survey project, -fields In STar forming RegiOns (BISTRO). The polarization vectors are used to identify the orientation of the magnetic field projected on the plane of the sky at a resolution of 0.01 pc. We identify 10 subregions with distinct polarization fractions and angles in the 0.2 pc ρ Oph-A core; some of them can be part of a coherent magnetic field structure in the ρ Oph region. The results are consistent with previous observations of the brightest regions of ρ Oph-A, where the degrees of polarization are at a level of a few percent, but our data reveal for the first time the magnetic field structures in the fainter regions surrounding the core where the degree of polarization is much higher (>5%). A comparison with previous near-infrared polarimetric data shows that there are several magnetic field components that are consistent at near-infrared and submillimeter wavelengths. Using the Davis–Chandrasekhar–Fermi method, we also derive magnetic field strengths in several subcore regions, which range from approximately 0.2 to 5 mG. We also find a correlation between the magnetic field orientations projected on the sky and the core centroid velocity components.

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 categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.727
Threshold uncertainty score1.000

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 studies0.0010.001
Scholarly communication0.0000.000
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 head0.031
GPT teacher head0.250
Teacher spread0.219 · 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.

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

Citations74
Published2018
Admission routes1
Has abstractyes

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