Show simple item record

Files in this item

Thumbnail

Item metadata

dc.contributor.authorLagatsky, A. A.
dc.contributor.authorKoopmann, P.
dc.contributor.authorFuhrberg, P.
dc.contributor.authorHuber, G.
dc.contributor.authorBrown, C. T. A.
dc.contributor.authorSibbett, W.
dc.date.accessioned2013-03-27T16:31:03Z
dc.date.available2013-03-27T16:31:03Z
dc.date.issued2012-02-01
dc.identifier.citationLagatsky , A A , Koopmann , P , Fuhrberg , P , Huber , G , Brown , C T A & Sibbett , W 2012 , ' Passively mode locked femtosecond Tm:Sc2O3 laser at 2.1 mu m ' , Optics Letters , vol. 37 , no. 3 , pp. 437-439 . https://doi.org/10.1364/OL.37.000437en
dc.identifier.issn0146-9592
dc.identifier.otherPURE: 27075609
dc.identifier.otherPURE UUID: ae6eb133-d23a-4738-8e26-96710b38d315
dc.identifier.otherWOS: 000300407600052
dc.identifier.otherScopus: 84856668782
dc.identifier.otherORCID: /0000-0002-4405-6677/work/86537120
dc.identifier.urihttps://hdl.handle.net/10023/3442
dc.descriptionThis work was supported by EPSRCen
dc.description.abstractWe report on the passive mode locking of a Tm3+:Sc2O3 laser at 2.1 mu m using a semiconductor saturable absorber mirror based on InGaAsSb quantum wells. Transform-limited 218 fs pulses are generated with an average power of 210 mW. A maximum output power of 325 mW is produced during mode locking with the corresponding pulse duration of 246 fs at a pulse repetition frequency of 124.3 MHz. A Ti:sapphire laser is used as the pump source operating at 796 nm. (C) 2012 Optical Society of America
dc.format.extent3
dc.language.isoeng
dc.relation.ispartofOptics Lettersen
dc.rights© 2012 Optical Society of America. This paper was published in Optics Letters and is made available as an electronic reprint with the permission of OSA. The paper can be found at http://www.opticsinfobase.orgen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titlePassively mode locked femtosecond Tm:Sc2O3 laser at 2.1 mu men
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1364/OL.37.000437
dc.description.statusPeer revieweden


This item appears in the following Collection(s)

Show simple item record