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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 OpenAlex
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

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.
aboutThe title or abstract carries a Canadian signal from the geographic lexicon.

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.

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 categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.915
Threshold uncertainty score0.999

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)0.0020.000

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 head0.005
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

Quick stats

Citations5
Published2024
Admission routes2
Has abstractyes

Explore more

Same topicHistory and Developments in AstronomyFrench-language works237,207