Evidence map›Paper›PMID 38368423›Full record

ArticleNature communications2024

Continuous ultraviolet to blue-green astrocomb.

Yuk Shan Cheng, Kamalesh Dadi, Toby Mitchell, Samantha Thompson, Nikolai Piskunov, Lewis D Wright, Corin B E Gawith, Richard A McCracken, Derryck T Reid

Open access · goldAbstract 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 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing papers in PubMed
4.1field-weighted citation impact, top 6% of its field
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

5 citing papers in PubMed, 12 citations in OpenAlex.

  1. Article
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  5. Review
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

9 authors at 4 institutions in 2 countries.

Yuk Shan ChengInstitute of Photonics and Quantum Sciences, Heriot-Watt University, Edinburgh, EH14 4AS, UK.
Kamalesh DadiInstitute of Photonics and Quantum Sciences, Heriot-Watt University, Edinburgh, EH14 4AS, UK.ORCID http://orcid.org/0009-0001-5668-9092
Toby MitchellInstitute of Photonics and Quantum Sciences, Heriot-Watt University, Edinburgh, EH14 4AS, UK.
Samantha ThompsonAstrophysics Group, Cavendish Laboratory, J.J. Thomson Avenue, Cambridge, CB3 0HE, UK.ORCID http://orcid.org/0000-0002-8039-194X
Nikolai PiskunovDepartment of Physics and Astronomy, Uppsala University, Box 516, 751 20, Uppsala, Sweden.
Lewis D WrightCovesion Ltd, Unit F3, Adanac North, Adanac Drive, Nursling, Southampton, SO16 0BT, UK.
Corin B E GawithCovesion Ltd, Unit F3, Adanac North, Adanac Drive, Nursling, Southampton, SO16 0BT, UK.ORCID http://orcid.org/0000-0002-3502-3558
Richard A McCrackenInstitute of Photonics and Quantum Sciences, Heriot-Watt University, Edinburgh, EH14 4AS, UK.ORCID http://orcid.org/0000-0002-9294-1910
Derryck T ReidInstitute of Photonics and Quantum Sciences, Heriot-Watt University, Edinburgh, EH14 4AS, UK. D.T.Reid@hw.ac.uk.ORCID http://orcid.org/0000-0002-0385-4939
Heriot-Watt University · GBCovesion (United Kingdom) · GBUniversity of Cambridge · GBUppsala University · SE

Funding

RCUK | Science and Technology Facilities Council (STFC) ST/N002997/1RCUK | Science and Technology Facilities Council (STFC) ST/S001328/1RCUK | Science and Technology Facilities Council (STFC) ST/V000403/1RCUK | Science and Technology Facilities Council (STFC) ST/V000918/1RCUK | Science and Technology Facilities Council (STFC) ST/X002306/1RCUK | Science and Technology Facilities Council (STFC) ST/Y001273/1Royal Academy of Engineering RCSRF1718639Royal Academy of Engineering RCSRF2223-1678
6 · The paper itself

Abstract

Cosmological and exoplanetary science using transformative telescopes like the ELT will demand precise calibration of astrophysical spectrographs in the blue-green, where stellar absorption lines are most abundant. Astrocombs-lasers providing a broadband sequence of regularly-spaced optical frequencies on a multi-GHz grid-promise an atomically-traceable calibration scale, but their realization in the blue-green is challenging for current infrared-laser-based technology. Here, we introduce a concept achieving a broad, continuous spectrum by combining second-harmonic generation and sum-frequency-mixing in an MgO:PPLN waveguide to generate 390-520 nm light from a 1 GHz Ti:sapphire frequency comb. Using a Fabry-Pérot filter, we extract a 30 GHz sub-comb spanning 392-472 nm, visualizing its thousands of modes on a high-resolution spectrograph. Experimental data and simulations demonstrate how the approach can bridge the spectral gap present in second-harmonic-only conversion. Requiring only [Formula: see text]100 pJ pulses, our concept establishes a new route to broadband UV-visible generation at GHz repetition rates.

Identifiers

PMID38368423
PMCPMC10874390
OpenAlexW4391899265

What OpenQuestion holds

Textmetadata
LicenceCC BY
Read underepoch 390

Registered trials

None linked

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.