% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@ARTICLE{Ludwig:612774,
author = {Ludwig, Markus and Ayhan, Furkan and Schmidt, Tobias M. and
Wildi, Thibault and Voumard, Thibault and Blum, Roman and
Ye, Zhichao and Lei, Fuchuan and Wildi, François and Pepe,
Francesco and Gaafar, Mahmoud A. and Obrzud, Ewelina and
Grassani, Davide and Moreau, François and Chazelas, Bruno
and Sottile, Rico and Torres-Company, Victor and Brasch,
Victor and Villanueva, Luis G. and Bouchy, François and
Herr, Tobias},
title = {{U}ltraviolet astronomical spectrograph calibration with
laser frequency combs from nanophotonic lithium niobate
waveguides},
journal = {Nature Communications},
volume = {15},
number = {1},
issn = {2041-1723},
address = {[London]},
publisher = {Nature Publishing Group UK},
reportid = {PUBDB-2024-05459},
pages = {7614},
year = {2024},
abstract = {Astronomical precision spectroscopy underpins searches for
life beyond Earth, direct observation of the expanding
Universe and constraining the potential variability of
physical constants across cosmological scales. Laser
frequency combs can provide the critically required accurate
and precise calibration to the astronomical spectrographs.
For cosmological studies, extending the calibration with
such astrocombs to the ultraviolet spectral range is highly
desirable, however, strong material dispersion and large
spectral separation from the established infrared laser
oscillators have made this exceedingly challenging. Here, we
demonstrate for the first time astronomical spectrograph
calibrations 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 may contribute to
unlocking the full potential of next generation ground- and
future space-based astronomical instruments.},
cin = {FS-CFEL-2-UMP},
ddc = {500},
cid = {I:(DE-H253)FS-CFEL-2-UMP-20201209},
pnm = {631 - Matter – Dynamics, Mechanisms and Control
(POF4-631) / STARCHIP - Microphotonics-based frequency combs
for habitable exoplanet detection (853564) / VH-NG-1404 -
Ultra-fast nonlinear microphotonics
$(G:(DE-HGF)2019_VH-NG-1404)$ / DarkComb - Dark-Soliton
Engineering in Microresonator Frequency Combs (771410)},
pid = {G:(DE-HGF)POF4-631 / G:(EU-Grant)853564 /
$G:(DE-HGF)2019_VH-NG-1404$ / G:(EU-Grant)771410},
experiment = {EXP:(DE-H253)CFEL-Exp-20150101},
typ = {PUB:(DE-HGF)16},
eprint = {2306.13609},
howpublished = {arXiv:2306.13609},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2306.13609;\%\%$},
pubmed = {39223131},
UT = {WOS:001304177200014},
doi = {10.1038/s41467-024-51560-x},
url = {https://bib-pubdb1.desy.de/record/612774},
}