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Record W2080163811 · doi:10.1088/0004-637x/768/1/55

<i>HERSCHEL</i>/SPIRE SUBMILLIMETER SPECTRA OF LOCAL ACTIVE GALAXIES<sup>,</sup>

2013· article· fr· W2080163811 on OpenAlexafffund
M. Pereira-Santaella, L. Spinoglio, G. Busquet, C. D. Wilson, Jason Glenn, K. G. Isaak, J. Kamenetzky, Naseem Rangwala, Maximilien R. P. Schirm, M. Baes, M. J. Barlow, Alessandro Boselli, Asantha Cooray, D. Cormier

Bibliographic record

VenueThe Astrophysical Journal · 2013
Typearticle
Languagefr
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsMcMaster University
FundersNational Astronomical Observatories, Chinese Academy of SciencesScience and Technology Facilities CouncilCentre National de la Recherche ScientifiqueImperial College LondonAgenzia Spaziale ItalianaUniversità degli Studi di PadovaJet Propulsion LaboratoryCentre National d’Etudes SpatialesCardiff UniversityUniversity of SussexNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyUniversity of LethbridgeUK Space Agency
KeywordsPhysicsGalaxyAstrophysicsSpire (mollusc)Spectral lineEmission spectrumRadiative transferLine (geometry)Luminous infrared galaxyStar formationMillimeterAstronomy

Abstract

fetched live from OpenAlex

We present the submillimeter spectra from 450 to 1550 GHz of 11 nearby active galaxies observed with the SPIRE Fourier Transform Spectrometer (SPIRE/FTS) on board Herschel . We detect CO transitions from J up = 4 to 12, as well as the two [C i ] fine structure lines at 492 and 809 GHz and the [N ii ]1461 GHz line. We used radiative transfer models to analyze the observed CO spectral line energy distributions. The FTS CO data were complemented with ground-based observations of the low- J CO lines. We found that the warm molecular gas traced by the mid- J CO transitions has similar physical conditions ( 10 3.2 –10 3.9 cm −3 and T kin ∼ 300–800 K) in most of our galaxies. Furthermore, we found that this warm gas is likely producing the mid-IR rotational H 2 emission. We could not determine the specific heating mechanism of the warm gas, however, it is possibly related to the star formation activity in these galaxies. Our modeling of the [C i ] emission suggests that it is produced in cold ( T kin < 30 K) and dense ( cm −3 ) molecular gas. Transitions of other molecules are often detected in our SPIRE/FTS spectra. The HF J = 1–0 transition at 1232 GHz is detected in absorption in UGC 05101 and in emission in NGC 7130. In the latter, near-infrared pumping, chemical pumping, or collisional excitation with electrons are plausible excitation mechanisms likely related to the active galactic nucleus of this galaxy. In some galaxies, few H 2 O emission lines are present. Additionally, three OH + lines at 909, 971, and 1033 GHz are identified in NGC 7130.

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)0.001
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: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.041
Threshold uncertainty score0.137

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0040.002
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0410.010

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 head0.217
Teacher spread0.208 · 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

Citations54
Published2013
Admission routes2
Has abstractyes

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