MétaCan
Menu
Back to cohort
Record W1994821728 · doi:10.1088/2041-8205/781/1/l15

<i>HERSCHEL</i> OBSERVATIONS OF FAR-INFRARED COOLING LINES IN INTERMEDIATE REDSHIFT (ULTRA)-LUMINOUS INFRARED GALAXIES

2014· article· en· W1994821728 on OpenAlexaff
D. Rigopoulou, R. Hopwood, G. Magdis, N. Thatte, B. M. Swinyard, D. Farrah, Jiasheng Huang, A. Alonso‐Herrero, J. Böck, D. L. Clements, Asantha Cooray, Matthew Griffin, Seb Oliver, Chris Pearson, Dominik A. Riechers, D. Scott, A. J. Smith, M. Vaccari, I. Valtchanov, L. Wang

Bibliographic record

VenueThe Astrophysical Journal Letters · 2014
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of British Columbia
FundersScience and Technology Facilities Council
KeywordsPhysicsAstrophysicsLuminous infrared galaxyRedshiftGalaxyStar formationAstronomyLuminosityInfrared

Abstract

fetched live from OpenAlex

We report the first results from a spectroscopic survey of the [C ii ] 158 μm line from a sample of intermediate redshift (0.2 < z < 0.8) (ultra)-luminous infrared galaxies, (U)LIRGs ( L IR > 10 11.5 L ☉ ), using the Spectral and Photometric Imaging REceiver–Fourier Transform Spectrometer on board the Herschel Space Observatory . This is the first survey of [C ii ] emission, an important tracer of star formation, at a redshift range where the star formation rate density of the universe increases rapidly. We detect strong [C ii ] 158 μm line emission from over 80% of the sample. We find that the [C ii ] line is luminous, in the range (0.8–4) × 10 −3 of the far-infrared continuum luminosity of our sources, and appears to arise from photodissociation regions on the surface of molecular clouds. The L [C ii ] / L IR ratio in our intermediate redshift (U)LIRGs is on average ∼10 times larger than that of local ULIRGs. Furthermore, we find that the L [C ii ] / L IR and L [C ii ] / L CO(1–0) ratios in our sample are similar to those of local normal galaxies and high- z star-forming galaxies. ULIRGs at z ∼ 0.5 show many similarities to the properties of local normal and high- z star-forming galaxies. Our findings strongly suggest that rapid evolution in the properties of the star-forming regions of (U)LIRGs is likely to have occurred in the last 5 billion years.

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 score0.004
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
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 head0.010
GPT teacher head0.208
Teacher spread0.198 · 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

Citations45
Published2014
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical Journal LettersSame topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207