Ultrafast laser inscription of asymmetric integrated waveguide 3 dB couplers for astronomical K-band interferometry at the CHARA array

dc.bibliographicCitation.firstPage2455eng
dc.bibliographicCitation.issue9eng
dc.bibliographicCitation.journalTitleJournal of the Optical Society of America : JOSA : B, Optical physicseng
dc.bibliographicCitation.lastPage2464eng
dc.bibliographicCitation.volume38eng
dc.contributor.authorBenoît, Aurélien
dc.contributor.authorPike, Fraser A.
dc.contributor.authorSharma, Tarun K.
dc.contributor.authorMacLachlan, David G.
dc.contributor.authorDinkelaker, Aline N.
dc.contributor.authorNayak, Abani S.
dc.contributor.authorMadhav, Kalaga
dc.contributor.authorRoth, Martin M.
dc.contributor.authorLabadie, Lucas
dc.contributor.authorPedretti, Ettore
dc.contributor.authorBrummelaar, Theo A. ten
dc.contributor.authorScott, Nic
dc.contributor.authorCoudé du Foresto, Vincent
dc.contributor.authorThomson, Robert R.
dc.date.accessioned2022-03-24T13:34:56Z
dc.date.available2022-03-24T13:34:56Z
dc.date.issued2021
dc.description.abstractWe present the fabrication and characterization of 3 dB asymmetric directional couplers for the astronomical K-band at wavelengths between 2.0 and 2.4 µm. The couplers were fabricated in commercial Infrasil silica glass using an ultrafast laser operating at 1030 nm. After optimizing the fabrication parameters, the insertion losses of straight single-mode waveguides were measured to be ∼1.2±0.5dB across the full K-band. We investigate the development of asymmetric 3 dB directional couplers by varying the coupler interaction lengths and by varying the width of one of the waveguide cores to detune the propagation constants of the coupled modes. In this manner, we demonstrate that ultrafast laser inscription is capable of fabricating asymmetric 3 dB directional couplers for future applications in K-band stellar interferometry. Finally, we demonstrate that our couplers exhibit an interferometric fringe contrast of >90%. This technology paves the path for the development of a two-telescope K-band integrated optic beam combiner for interferometry to replace the existing beam combiner (MONA) in Jouvence of the Fiber Linked Unit for Recombination (JouFLU) at the Center for High Angular Resolution Astronomy (CHARA) telescope array.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/8364
dc.identifier.urihttps://doi.org/10.34657/7402
dc.language.isoengeng
dc.publisherWashington, DC : Soc.eng
dc.relation.doihttps://doi.org/10.1364/JOSAB.423727
dc.relation.essn1520-8540
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subject.ddc530eng
dc.subject.ddc620eng
dc.subject.otherDirectional couplerseng
dc.subject.otherElectric losseseng
dc.subject.otherFabricationeng
dc.subject.otherInterferometryeng
dc.subject.otherSilicaeng
dc.subject.otherTelescopeseng
dc.subject.other3 dB directional couplerseng
dc.subject.otherFabrication and characterizationseng
dc.subject.otherFabrication parameterseng
dc.subject.otherHigh angular resolutionseng
dc.subject.otherIntegrated waveguideseng
dc.subject.otherInterferometric fringeseng
dc.subject.otherSingle mode waveguideseng
dc.subject.otherStellar interferometryeng
dc.subject.otherUltrafast laserseng
dc.titleUltrafast laser inscription of asymmetric integrated waveguide 3 dB couplers for astronomical K-band interferometry at the CHARA arrayeng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccesseng
wgl.contributorAIPeng
wgl.subjectPhysikeng
wgl.typeZeitschriftenartikeleng
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