Evidence map›Paper›PMID 39223131›Full record

ArticleNature communications2024

Ultraviolet astronomical spectrograph calibration with laser frequency combs from nanophotonic lithium niobate waveguides.

Markus Ludwig, Furkan Ayhan, Tobias M Schmidt, Thibault Wildi, Thibault Voumard, Roman Blum, Zhichao Ye, Fuchuan Lei, François Wildi, Francesco Pepe and 14 more

Abstract read
In one paragraph

Article in Nature communications, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 6 papers.

0numbers the graph read from it
0cells of the map it votes in
6citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

6 citing papers in PubMed.

  1. Article
  2. Article
  3. Article
  4. Femtosecond pulse amplification on a chip.Nature communications · 2024
    Article
  5. Article
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4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

24 authors.

Markus Ludwig *Deutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607, Hamburg, Germany.
Furkan Ayhan *École Polytechnique Fédérale de Lausanne (EPFL), 1015, Lausanne, Switzerland.ORCID http://orcid.org/0000-0001-6606-0709
Tobias M Schmidt *Observatoire de Genève, Département d'Astronomie, Université de Genève, Chemin Pegasi 51b, 1290, Versoix, Switzerland.ORCID http://orcid.org/0000-0002-4833-7273
Thibault WildiDeutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607, Hamburg, Germany.ORCID http://orcid.org/0000-0002-0193-7132
Thibault VoumardDeutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607, Hamburg, Germany.
Roman BlumSwiss Center for Electronics and Microtechnology (CSEM), 2000, Neuchâtel, Switzerland.
Zhichao YeDepartment of Microtechnology and Nanoscience, Chalmers University of Technology, 41296, Gothenburg, Sweden.ORCID http://orcid.org/0000-0002-4708-3582
Fuchuan LeiDepartment of Microtechnology and Nanoscience, Chalmers University of Technology, 41296, Gothenburg, Sweden.ORCID http://orcid.org/0000-0003-2257-7057
François WildiObservatoire de Genève, Département d'Astronomie, Université de Genève, Chemin Pegasi 51b, 1290, Versoix, Switzerland.
Francesco PepeObservatoire de Genève, Département d'Astronomie, Université de Genève, Chemin Pegasi 51b, 1290, Versoix, Switzerland.
Mahmoud A GaafarDeutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607, Hamburg, Germany.ORCID http://orcid.org/0000-0001-5887-5772
Ewelina ObrzudSwiss Center for Electronics and Microtechnology (CSEM), 2000, Neuchâtel, Switzerland.
Davide GrassaniSwiss Center for Electronics and Microtechnology (CSEM), 2000, Neuchâtel, Switzerland.
Olivia HeftiSwiss Center for Electronics and Microtechnology (CSEM), 2000, Neuchâtel, Switzerland.
Sylvain KarlenSwiss Center for Electronics and Microtechnology (CSEM), 2000, Neuchâtel, Switzerland.ORCID http://orcid.org/0000-0001-8404-6521
Steve LecomteSwiss Center for Electronics and Microtechnology (CSEM), 2000, Neuchâtel, Switzerland.
François MoreauObservatoire de Haute-Provence, CNRS, Université d'Aix-Marseille, 04870, Saint-Michel-l'Observatoire, France.
Bruno ChazelasObservatoire de Genève, Département d'Astronomie, Université de Genève, Chemin Pegasi 51b, 1290, Versoix, Switzerland.
Rico SottileObservatoire de Haute-Provence, CNRS, Université d'Aix-Marseille, 04870, Saint-Michel-l'Observatoire, France.
Victor Torres-CompanyDepartment of Microtechnology and Nanoscience, Chalmers University of Technology, 41296, Gothenburg, Sweden.ORCID http://orcid.org/0000-0002-3504-2118
Victor BraschQ.ANT GmbH, Handwerkstraße 29, 70565, Stuttgart, Germany.ORCID http://orcid.org/0000-0002-0354-2847
Luis G VillanuevaÉcole Polytechnique Fédérale de Lausanne (EPFL), 1015, Lausanne, Switzerland.ORCID http://orcid.org/0000-0003-3340-2930
François BouchyObservatoire de Genève, Département d'Astronomie, Université de Genève, Chemin Pegasi 51b, 1290, Versoix, Switzerland.
Tobias HerrDeutsches Elektronen-Synchrotron DESY, Notkestr. 85, 22607, Hamburg, Germany. tobias.herr@desy.de.ORCID http://orcid.org/0000-0002-5966-6697

Funding

Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung (Swiss National Science Foundation) CRSII5 193689
6 · The paper itself

Abstract

Astronomical precision spectroscopy underpins searches for life beyond Earth, direct observation of the expanding Universe and constraining the potential variability of physical constants on cosmological scales. Laser frequency combs can provide the required accurate and precise calibration to the astronomical spectrographs. For cosmological studies, extending the calibration with such astrocombs to the ultraviolet spectral range is desirable, however, strong material dispersion and large spectral separation from the established infrared laser oscillators have made this challenging. Here, we demonstrate astronomical spectrograph calibration with an astrocomb in the ultraviolet spectral range below 400 nm. This is accomplished via chip-integrated highly nonlinear photonics in periodically-poled, nano-fabricated lithium niobate waveguides in conjunction with a robust infrared electro-optic comb generator, as well as a chip-integrated microresonator comb. These results demonstrate a viable route towards astronomical precision spectroscopy in the ultraviolet and could contribute to unlock the full potential of next-generation ground-based and future space-based instruments.

Identifiers

PMID39223131
PMCPMC11369296

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Registered trials

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.