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dc.contributor.authorObrzud, Ewelina
dc.contributor.authorRainer, Monica
dc.contributor.authorHarutyunyan, Avet
dc.contributor.authorAnderson, Miles H.
dc.contributor.authorLiu, Junqiu
dc.contributor.authorGeiselmann, Michael
dc.contributor.authorChazelas, Bruno
dc.contributor.authorKundermann, Stefan
dc.contributor.authorLecomte, Steve
dc.contributor.authorCecconi, Massimo
dc.contributor.authorGhedina, Adriano
dc.contributor.authorMolinari, Emilio
dc.contributor.authorPepe, Francesco
dc.contributor.authorWildi, François
dc.contributor.authorBouchy, François
dc.contributor.authorKippenberg, Tobias J.
dc.contributor.authorHerr, Tobias
dc.date.accessioned2022-02-14T17:08:11Z
dc.date.available2022-02-14T17:08:11Z
dc.date.issued2019-01
dc.identifier.citationNature Photonics, vol. 13 (1), pp. 31
dc.identifier.issn1749-4893
dc.identifier.urihttps://yoda.csem.ch/handle/20.500.12839/924
dc.description.abstractA microphotonic astrocomb is demonstrated via temporal dissipative Kerr solitons in photonic-chip-based silicon nitride microresonators with a precision of 25?cm?s–1 (radial velocity equivalent), useful for Earth-like planet detection and cosmological research.
dc.titleA microphotonic astrocomb
dc.typeJournal Article
dc.type.csemdivisionsDiv-E
dc.type.csemresearchareasScientific Instrumentation
dc.type.csemresearchareasPhotonics
dc.identifier.urlhttps://www.nature.com/articles/s41566-018-0309-y
dc.identifier.doi10.1038/s41566-018-0309-y


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