MétaCan
Menu
Back to cohort
Record W2023263280 · doi:10.1051/0004-6361:20030344

Low upper limits on the O<sub>2</sub>abundance from the Odin satellite

2003· article· en· W2023263280 on OpenAlexafffund
L. Pagani, A. O. H. Olofsson, P. Bergman, P. F. Bernath, J. H. Black, R. S. Booth, V. Buat, J. Crovisier, Charles L. Curry, P. Encrenaz, É. Falgarone, P. A. Feldman, M. Fich, H.-G. Florén, U. Frisk, M. Gerin, E. M. Gregersen, J. Harju, T. Hasegawa, Åke Hjalmarson, L. E. B. Johansson, Sun Kwok, Bengt Larsson, A. Lecacheux, T. Liljeström, M. Lindqvist, R. Liseau, K. Mattila, G. F. Mitchell, L. Nordh, M. Olberg, G. Olofsson, I. Ristorcelli, Aa. Sandqvist, F. von Schéele, G. Serra, N. F. H. Tothill, Kevin Volk, Tommy Wiklind, C. D. Wilson

Bibliographic record

VenueAstronomy and Astrophysics · 2003
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Star Formation Studies
Canadian institutionsSaint Mary's UniversityUniversity of CalgaryMcMaster UniversityHerzberg Institute of AstrophysicsUniversity of Waterloo
FundersCanadian Space AgencyTekesCentre National d’Etudes Spatiales
KeywordsOutflowSatellitePhysicsExcited stateAstrophysicsAstronomyAtomic physicsMeteorology

Abstract

fetched live from OpenAlex

For the first time, a search has been conducted in our Galaxy for the 119 GHz transition connecting to the ground state of O2, using the Odin satellite. Equipped with a sensitive 3 mm receiver ( K), Odin has reached unprecedented upper limits on the abundance of O2, especially in cold dark clouds where the excited state levels involved in the 487 GHz transition are not expected to be significantly populated. Here we report upper limits for a dozen sources. In cold dark clouds we improve upon the published SWAS upper limits by more than an order of magnitude, reaching N(O2)/N(H in half of the sources. While standard chemical models are definitively ruled out by these new limits, our results are compatible with several recent studies that derive lower O2 abundances. Goldsmith et al. (2002) recently reported a SWAS tentative detection of the 487 GHz transition of O2 in an outflow wing towards ρ Oph A in a combination of 7 beams covering approximately . In a brief (1.3 hour integration time) and partial covering of the SWAS region (≈65% if we exclude their central position), we did not detect the corresponding 119 GHz line. Our 3 sigma upper limit on the O2 column density is cm-2. We presently cannot exclude the possibility that the SWAS signal lies mostly outside of the 9´ Odin beam and has escaped our sensitive detector.

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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.641
Threshold uncertainty score0.917

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 studies0.0010.000
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 head0.009
GPT teacher head0.196
Teacher spread0.186 · 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.

The models applied no category: nothing in the taxonomy fit this work.
Study designNot applicable
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

Citations107
Published2003
Admission routes2
Has abstractyes

Explore more

Same venueAstronomy and AstrophysicsSame topicAstrophysics and Star Formation StudiesFrench-language works237,207