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A search for neutral carbon towards two<i>z</i>= 4.05 submillimetre galaxies, GN���20 and GN���20.2

2009· article· en· W2070101788 on OpenAlexaff
Caitlin M. Casey, S. C. Chapman, E. Daddi, H. Dannerbauer, Alexandra Pope, D. Scott, F. Bertoldi, R. J. Beswick, A. W. Blain, P. Cox, R. Genzel, T. R. Greve, R. J. Ivison, T. W. B. Muxlow, R. Neri, A. Omont, Ian Smail, L. J. Tacconi

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2009
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of British Columbia
FundersCentre National de la Recherche ScientifiqueCambridge TrustScience and Technology Facilities CouncilMax-Planck-GesellschaftAgence Nationale de la Recherche
KeywordsPhysicsPlateau de Bure InterferometerAstrophysicsGalaxyRedshiftLuminosityAtomic carbonLuminous infrared galaxyMilky WayLine (geometry)Hydrogen

Abstract

fetched live from OpenAlex

Using the IRAM Plateau de Bure Interferometer (PdBI) we have searched for the upper fine structure line of neutral carbon [] and 12CO(J= 7 → 6) (νrest= 806 GHz) towards the submillimetre galaxies (SMGs) GN 20 (SMM J123711.9+622212, z= 4.055) and GN 20.2 (SMM J123708.8+622202, z= 4.051). The far-infrared continuum is detected at 8σ significance in GN 20, with a flux density of S1.8 mm= 1.9 ± 0.2 mJy, while no continuum is detected in GN 20.2. Both sources are statistically undetected in both and 12CO(J= 7 → 6) lines; we derive line luminosity limits for both C i and CO of L′≲ 2 × 1010 K km s−1 pc2. Assuming carbon excitation temperatures of Tex= 30 K (the galaxies' measured dust temperatures), we infer C i mass limits of MC i < 5.4 × 106 M⊙ (GN 20) and MC i < 6.8 × 106 M⊙ (GN 20.2). The derived C i abundance limits are <1.8 × 10−5 for GN 20 and <3.8 × 10−5 for GN 20.2, implying that the systems have Milky Way level carbon enrichment (X[C i]/X[H2]) or lower, similar to high-redshift carbon-detected systems (at 5 × 10−5) but about 50 times less than the carbon enrichment of local starburst galaxies. Observations of GN 20 and GN 20.2 in high-resolution MERLIN+VLA (Multi-Element Radio Linked Interferometer Network+Very Large Array) radio maps of GOODS-N (Great Observatories Origin Deep Survey-North) are used to further constrain the sizes and locations of active regions. We conclude that the physical gas properties of young rapidly evolving systems like GN 20 and GN 20.2 are likely significantly different than starburst/ULIRG (ultraluminous infrared galaxy) environments in the local Universe yet similar to z∼ 2 SMGs. Unless gravitationally amplified examples can be found, observations of galaxies like GN 20 will require the order of magnitude increase in sensitivity of the Atacama Large Millimetre Array (ALMA) to constrain their C i and high-J CO content, despite the fact that they are the brightest systems at z∼ 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)0.000
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: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.009
Threshold uncertainty score0.018

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
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 head0.009
GPT teacher head0.216
Teacher spread0.207 · 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

Citations21
Published2009
Admission routes1
Has abstractyes

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