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Record W2942440081 · doi:10.1093/mnras/stz1215

Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum

2019· article· en· W2942440081 on OpenAlexfundno aff
A. Collier Cameron, Annelies Mortier, David F. Phillips, X. Dumusque, R. D. Haywood, Nicholas Langellier, C. A. Watson, H. M. Cegla, Jean C Costes, D. Charbonneau, A. Coffinet, David W. Latham, Mercedes López‐Morales, L. Malavolta, J. Maldonado, G. Micela, Timothy Milbourne, E. Molinari, Steven H. Saar, Samantha Thompson, N. Buchschacher, M. Cecconi, R. Cosentino, A. Ghedina, Alexander G. Glenday, Manuel Gonzalez, C.-H. Li, Marcello Lodi, C. Lovis, F. Pepe, E. Poretti, Ken Rice, Dimitar Sasselov, A. Sozzetti, Andrew Szentgyorgyi, S. Udry, Ronald L. Walsworth

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersHeliophysics DivisionScience and Technology Facilities CouncilSeventh Framework ProgrammeSmithsonian Astrophysical ObservatoryJet Propulsion LaboratoryUniversité de GenèveUniversity of EdinburghQueen's University BelfastUK Space AgencyUniversity of St AndrewsScottish Universities Physics AllianceCalifornia Institute of TechnologyEuropean CommissionQueen's UniversitySchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungNASA Exoplanet Science InstituteSchweizerische Zahnärzte-GesellschaftNational Aeronautics and Space AdministrationHarvard UniversitySmithsonian InstitutionNational Science Foundation
KeywordsPhysicsRadial velocityAstrophysicsAmplitudePlanetPlanetary systemAstronomyStarsOptics

Abstract

fetched live from OpenAlex

Abstract The time-variable velocity fields of solar-type stars limit the precision of radial-velocity determinations of their planets’ masses, obstructing detection of Earth twins. Since 2015 July, we have been monitoring disc-integrated sunlight in daytime using a purpose-built solar telescope and fibre feed to the HARPS-N stellar radial-velocity spectrometer. We present and analyse the solar radial-velocity measurements and cross-correlation function (CCF) parameters obtained in the first 3 yr of observation, interpreting them in the context of spatially resolved solar observations. We describe a Bayesian mixture-model approach to automated data-quality monitoring. We provide dynamical and daily differential-extinction corrections to place the radial velocities in the heliocentric reference frame, and the CCF shape parameters in the sidereal frame. We achieve a photon-noise-limited radial-velocity precision better than 0.43 m s−1 per 5-min observation. The day-to-day precision is limited by zero-point calibration uncertainty with an RMS scatter of about 0.4 m s−1. We find significant signals from granulation and solar activity. Within a day, granulation noise dominates, with an amplitude of about 0.4 m s−1 and an autocorrelation half-life of 15 min. On longer time-scales, activity dominates. Sunspot groups broaden the CCF as they cross the solar disc. Facular regions temporarily reduce the intrinsic asymmetry of the CCF. The radial-velocity increase that accompanies an active-region passage has a typical amplitude of 5 m s−1 and is correlated with the line asymmetry, but leads it by 3 d. Spectral line-shape variability thus shows promise as a proxy for recovering the true radial velocity.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.111
Threshold uncertainty score0.489

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 studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
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 head0.018
GPT teacher head0.203
Teacher spread0.185 · 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 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

Citations142
Published2019
Admission routes1
Has abstractyes

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