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Record W4210392977 · doi:10.1093/mnras/stac150

The bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the <i>Herschel</i> ATLAS

2022· article· en· W4210392977 on OpenAlexafffund
S. Urquhart, G. J. Bendo, S. Serjeant, Tom J. L. C. Bakx, Masato Hagimoto, P. Cox, R. Neri, M. D. Lehnert, Chris Sedgwick, Charles Weiner, H. Dannerbauer, Aristeidis Amvrosiadis, P. Andreani, A. J. Baker, A. Beelen, S. Berta, E. Borsato, V. Buat, K. Butler, Asantha Cooray, G. de Zotti, L. Dunne, S. Dye, S. Eales, A Enia, Lulu Fan, R. Gavazzi, J. González-Nuevo, A. I. Harris, Cinthya N. Herrera, D. H. Hughes, D. Ismail, R. J. Ivison, Shuowen Jin, B. Jones, Kotaro Kohno, M. Krips, G. Lagache, L. Marchetti, M. Massardi, Hugo Messias, M. Negrello, A. Omont, I. Pérez‐Fournon, Dominik A. Riechers, D. Scott, M. W. L. Smith, F. Stanley, Yoichi Tamura, P. Temi, C. Vlahakis, A. Weiß, P. van der Werf, A. Verma, C. Yang, A. J. Young

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of British Columbia
FundersAgencia Estatal de InvestigaciónNational Astronomical Observatory of JapanScience and Technology Facilities CouncilMinistero dell’Istruzione, dell’Università e della RicercaFederación Española de Enfermedades RarasAgencia Canaria de Investigación, Innovación y Sociedad de la InformaciónMinisterio de Ciencia e InnovaciónAlberta Livestock and Meat AgencyEuropean School of OncologyEuropean Regional Development FundEuropean CommissionJapan Society for the Promotion of ScienceHorizon 2020 Framework ProgrammeMinistry of Science and TechnologyNational Science FoundationU.S. Nuclear Regulatory CommissionAeroDynamic SolutionsDeutsche ForschungsgemeinschaftAgence Nationale de la RechercheNational Institutes of Natural SciencesAlbert Ellis InstituteKorea Astronomy and Space Science InstituteNational Aeronautics and Space Administration
KeywordsPhysicsRedshiftAstrophysicsGalaxyAstronomyRedshift surveyAtlas (anatomy)Submillimeter ArrayStar formation

Abstract

fetched live from OpenAlex

ABSTRACT We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimetre sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimize its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range 1.41 < z < 4.53 with a mean value of 2.75, and the CO emission line full-width at half-maxima range between $\rm 110\, km\, s^{-1} \lt FWHM \lt 1290\, km\, s^{-1}$ with a mean value of ∼500 km s−1, in line with other high-z samples. The derived CO(1-0) luminosity is significantly elevated relative to line-width to CO(1-0) luminosity scaling relation, which is suggestive of lensing magnification across our sources. In fact, the distribution of magnification factors inferred from the CO equivalent widths is consistent with expectations from galaxy–galaxy lensing models, though there is a hint of an excess at large magnifications that may be attributable to the additional lensing optical depth from galaxy groups or clusters.

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)0.001
metaresearch head score (Gemma)0.001
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 score0.008
Threshold uncertainty score0.017

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.001

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 head0.009
GPT teacher head0.199
Teacher spread0.190 · 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

Citations32
Published2022
Admission routes2
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→