MétaCan
Menu
Back to cohort
Record W4400725004 · doi:10.1117/12.3018994

NIRPS first light and early science: breaking the 1 m/s RV precision barrier at infrared wavelengths

2024· article· en· W4400725004 on OpenAlexaffabout
Étienne Artigau, F. Bouchy, René Doyon, Frédérique Baron, Lison Malo, F. Wildi, Franceso Pepe, Neil J. Cook, Simon Thibault, В. А. Решетов, X. Dumusque, C. Lovis, Danuta Sosnowska, B. L. Canto Martins, J. R. De Medeiros, X. Delfosse, N. C. Santos, R. Rébolo, Manuel Abreu, Guillaume Allain, Romain Allart, Hugues Auger, S. C. C. Barros, Luc Bazinet, Nicolas Blind, Isabelle Boisse, X. Bonfıls, V. Bourrier, Sébastien Bovay, C. Broeg, Denis Brousseau, Vincent Bruniquel, Alexandre Cabral, Charles Cadieux, A. Carmona, Yann Carteret, Zalpha Challita, Bruno Chazelas, Ryan Cloutier, João Coelho, Marion Cointepas, Uriel Conod, Nicolas B. Cowan, E. Cristo, J. Gomes da Silva, Laurie Dauplaise, Roseane Lima Gomes, E. Delgado Mena, D. Ehrenreich, J. P. Faria, P. Figueira, T. Forveille, Yolanda G. C. Frensch, Jonathan Gagné, Frédéric Genest, Ludovic Genolet, J. I. Gónzalez Hernández, Félix Gracia Témich, Nolan Grieves, Olivier Hernandez, Mélissa J. Hobson, H. J. Hoeijmakers, Dan Kerley, Vigneshwaran Krishnamurthy, David Lafrenière, Pierrot Lamontagne, Pierre Larue, Henry Leaf, I. C. Leão, Olivia Lim, G. Lo Curto, Allan Martins, Claudio Melo, Yuri S. Messias, L. Mignon, Leslie Moranta, C. Mordasini, Khaled Al Moulla, Dany Mounzer, Alexandrine L’Heureux, N. Nari, Louise Nielsen, Ares Osborn, Léna Parc, Luca Pasquini, V. M. Passegger, Stefan Pelletier, Céline Péroux, Caroline Piaulet, Mykhaylo Plotnykov, Anne-Sophie Poulin-Girard, José Luis Rasilla, Jonathan Saint-Antoine, Mirsad Sarajic, Alex Segovia, J. V. Seidel, D. Ségransan, Ana Rita Silva, Avidaan Srivastava, Atanas K. Stefanov, A. Suárez Mascareño, Michaël Sordet, Márcio A. Teixeira, S. Udry, Diana Valencia, Philippe Vallée, Thomas Vandal, Valentina Vaulato, Gregg Wade, Joost P. Wardenier, Bachar Wehbé, Drew Weisserman, Ivan Wevers, Gérard Zins

Bibliographic record

Venuenot available
Typearticle
Languageen
FieldPhysics and Astronomy
TopicHistory and Developments in Astronomy
Canadian institutionsUniversité LavalHerzberg Institute of AstrophysicsUniversité de Montréal
Fundersnot available
KeywordsWavelengthInfraredOptoelectronicsOpticsPhysicsMaterials science

Abstract

fetched live from OpenAlex

The Near-InfraRed Planet Searcher or NIRPS is a precision radial velocity spectrograph developed through collaborative efforts among laboratories in Switzerland, Canada, Brazil, France, Portugal and Spain. NIRPS extends to the 0.98-1.8 μm domain of the pioneering HARPS instrument at the La Silla 3.6-m telescope in Chile and it has achieved unparalleled precision, measuring stellar radial velocities in the infrared with accuracy better than 1 m/s. NIRPS can be used either standalone, or simultaneously with HARPS. Commissioned in late 2022 and early 2023, NIRPS embarked on a 5-year Guaranteed Time Observation (GTO) program in April 2023, spanning 720 observing nights. This program focuses on planetary systems around M dwarfs, encompassing both the immediate solar vicinity and transit follow-ups, alongside transit and emission spectroscopy observations. We highlight NIRPS’s current performances and the insights gained during its deployment at the telescope. The lessons learned and successes achieved contribute to the ongoing advancement of precision radial velocity measurements and high spectral fidelity, further solidifying NIRPS’ role in the forefront of the field of exoplanets.

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)0.007
metaresearch head score (Gemma)0.011
Version: metacan-v3-hybrid-931329e0061cValidation 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: none
Teacher disagreement score0.007
Threshold uncertainty score0.039

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0070.011
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.002
Scholarly communication0.0030.005
Open science0.0010.006
Research integrity0.0010.005
Insufficient payload (model declined to judge)0.0040.003

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 head0.005
GPT teacher head0.223
Teacher spread0.218 · 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 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

Citations5
Published2024
Admission routes2
Has abstractyes

Explore more

Same topicHistory and Developments in AstronomyFrench-language works237,207