Searching for p-modes in n Boötis & Procyon using MOST satellite data. Veröffentlichungen der Kommission für Astronomie|Communications in Asteroseismology|Communications in Asteroseismology 151 151|
Bibliographic record
Abstract
Die Serie Communications in Asteroseismology (CoAst) stellt eine international gefragte Plattform für wissenschaftliche Publikationen der neuesten Forschungsergebnisse auf dem Gebiet der Asteroseismologie dar. Forschungsgegenstand der Asteroseismologie sind veränderliche und pulsierende Sterne. Neben den halbjährlich erscheinenden regulären Ausgaben mit Beiträgen aus der laufenden Forschung werden auch Sonderausgaben für Konferenzberichte bzw. Programmhandbücher herausgegeben. Die Arbeiten in Vol.151 berichten über ein breites Spektrum der asteroseismologischen Forschung: Neben Beiträgen über die erdgebundene photometrische sowie spektroskopische Beobachtung von pulsierenden Sternen werden auch die neuesten Ergebnisse aus den Beobachtungen mit dem MOST-Satelliten besprochen. Theoretische Arbeiten über Konvektion und Opazitäten ergänzen diese Ausgabe. Contents: D. B. Guenther, T. Kallinger, P. Reegen, W. W. Weiss, J. M. Matthews, R. Kuschnig, A. F. J. Moffat, S. M. Rucinski, D. Sasselov and G. A. H. Walker: Searching for ρ-modes in η Boötis & Procyon using MOST satellite data; L. Fox Machado; J. H. Peña, G. Muñoz and B. Vargas: On the nature of the δ Scuti star star HD 115520; D. Sinachopoulos and P. Gavras: Photometric observations and frequency analysis of the δ Scuti NT Hya; J. C. Suárez, E. Michel, G. Houdek, F. Pérez Hernández and Y. Lebreton: Asteroseismology of δ Scuti Stars in open clusters: Praesepe; J. C. Suárez, R. Garrido and A. Moya: Analysis of II1/0 (Ω) period ratios in the presence of near degeneracy; A. Miglio, J. Montalbán and M.-A. Dupret: Revised instability domains of SPB and β Cephei stars; P. J. Amado: Near infrared spectroscopy of the HADS stars V703 Sco and 1 Mon: First steps towards the use of near-IR spectroscopy for the study of δ Scuti stars; C. Schoenaers and A. E. Lynas-Gray: A new slowly pulsating subdwarf-B star: HD 4539; M. Breger and P. Beck: Call for papers for the next issue of CoAst
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 imitationNot 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.
Distilled classifier scores by category (both heads)
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.000 | 0.000 |
| Meta-epidemiology (narrow) | 0.000 | 0.000 |
| Meta-epidemiology (broad) | 0.000 | 0.000 |
| Bibliometrics | 0.001 | 0.001 |
| Science and technology studies | 0.000 | 0.000 |
| Scholarly communication | 0.000 | 0.000 |
| Open science | 0.000 | 0.000 |
| Research integrity | 0.000 | 0.000 |
| Insufficient payload (model declined to judge) | 0.017 | 0.006 |
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.
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from itClassification
machine, unvalidatedMachine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.
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".