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Record W3055086379 · doi:10.1093/mnras/staa2569

SPIRou: NIR velocimetry and spectropolarimetry at the CFHT

2020· article· en· W3055086379 on OpenAlexaffabout
J.‐F. Donati, Driss Kouach, C. Moutou, René Doyon, X. Delfosse, Étienne Artigau, Sébastien Baratchart, M. Lacombe, Gregory Barrick, G. Hébrard, F. Bouchy, Les Saddlemyer, L. Parès, Patrick Rabou, Yoan Micheau, F. Dolon, В. А. Решетов, Zalpha Challita, A. Carmona, Nicolas Striebig, Simon Thibault, Eder Martioli, Neil J. Cook, P. Fouqué, Tom Vermeulen, Shiang‐Yu Wang, L. Arnold, F. Pepe, I. Boisse, P. Figueira, J. Bouvier, T. P. Ray, C Feugeade, J. Morin, S. H. P. Alencar, Mélissa J. Hobson, B. V. Castilho, S. Udry, N. C. Santos, Olivier Hernandez, Tom Benedict, Philippe Vallée, G. Gallou, M. Dupieux, Marie Larrieu, S. Perruchot, R. Sottile, F. Moreau, C. Usher, Marc Baril, F. Wildi, Bruno Chazelas, Lison Malo, X. Bonfıls, David Loop, Dan Kerley, Ivan Wevers, Jennifer Dunn, John Pazder, S. D. MacDonald, Bruno Dubois, Emilien Carrié, Hervé Valentín, François Hénault, T. Steinmetz

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsRio Tinto (Canada)Université LavalHerzberg Institute of AstrophysicsUniversité de Montréal
FundersFederación Española de Enfermedades RarasHorizon 2020 Framework ProgrammeCentre National de la Recherche ScientifiqueFundação para a Ciência e a TecnologiaH2020 European Research CouncilAgence Nationale de la Recherche
KeywordsPhysicsExoplanetAstronomyGravitational microlensingTelescopePlanetPlanetary systemSkyAtmosphere (unit)StarsVery Large TelescopeAstrobiologyAstrophysicsMeteorology

Abstract

fetched live from OpenAlex

ABSTRACT This paper presents an overview of SPIRou, the new-generation near-infrared spectropolarimeter/precision velocimeter recently installed on the 3.6-m Canada–France–Hawaii Telescope (CFHT). Starting from the two main science goals, i.e., the quest for planetary systems around nearby M dwarfs and the study of magnetized star/planet formation, we outline the instrument concept that was designed to efficiently address these forefront topics, and detail the in-lab and on-sky instrument performances measured throughout the intensive testing phase that SPIRou was submitted to before passing the final acceptance review in early 2019 and initiating science observations. With a central position among the newly started programmes, the SPIRou Legacy Survey (SLS) Large Programme was allocated 300 CFHT nights until at least mid 2022. We also briefly describe a few of the first results obtained in the various science topics that SPIRou started investigating, focusing in particular on planetary systems of nearby M dwarfs, transiting exoplanets and their atmospheres, magnetic fields of young stars, but also on alternate science goals like the atmospheres of M dwarfs and the Earth’s atmosphere. We finally conclude on the key role that SPIRou and the CFHT can play in coordination with forthcoming major facilities like the JWST, the ELTs, PLATO, and ARIEL over the decade.

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)0.003
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: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.012
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0030.002

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 head0.008
GPT teacher head0.198
Teacher spread0.189 · 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 designBench or experimental
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

Citations167
Published2020
Admission routes2
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical SocietySame topicStellar, planetary, and galactic studiesFrench-language works237,207