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dc.contributor.authorYu, Qingshan
dc.date.accessioned2024-08-23T00:45:13Z
dc.date.available2024-08-23T00:45:13Z
dc.date.issued2023en_AU
dc.identifier.urihttps://hdl.handle.net/2123/32984
dc.descriptionIncludes publication
dc.description.abstractAstrophotonics is a beautiful combination of the knowledge of photonics and astronomy. It offers the astronomy community unprecedented access to nanoscale light manipulation. In this thesis, I utilized established astrophotonics techniques such as photonic lanterns, and extended the capability of one specific technique - the AFBG OH suppression filters, into the astronomy J band. The achievements can be summarized as follows. - I explored the inscription of (A)FBGs into two types of 7-core fibers — trench-assisted and non-trench 7-core fibers. The results showed a slight reduction in wavelength offsets in the trench-assisted fibers, which may be attributed to the suppression of core-to-core coupling by the low-index trench. This will require further investigations. We plan to develop a Sagnac-type inscription rig to enable a core-by-core multicore FBG inscription method. - I proposed a complete design procedure for OH suppression AFBG filters, including detailed analysis of the OH Lambda doublets, detuning curve of the inscription setup and simplified optimization methods. I applied the procedure to the first J-band OH suppression AFBG filters and presented the fabrication results. These demonstrated the potential for AFBGs to be applied to any wavelength band within the J and H bands. - I proposed a detailed optimization method for the OH suppression AFBG design using artificial neural networks. The optimization method utilized a neural network based forward solver and a genetic algorithm. This novel approach offers the advantage of efficient implementation, requiring reduced computational time and resources, while yielding optimization outcomes of comparable quality to previous methods. - I built and tested the first J-band OH suppression unit consisting of 3 J-band AFBGs. This will be the beginning of the construction of a J-band OH suppressed spectrograph for celestial Positronium detection.en_AU
dc.language.isoenen_AU
dc.subjectAstrophotonicsen_AU
dc.subjectFBGen_AU
dc.subjectOH suppressionen_AU
dc.subjectastronomyen_AU
dc.subjectinstrumentationen_AU
dc.subjectspectrographen_AU
dc.titleFBGs in Specialty Optical Fibres for Astrophotonicsen_AU
dc.typeThesis
dc.type.thesisDoctor of Philosophyen_AU
dc.rights.otherThe author retains copyright of this thesis. It may only be used for the purposes of research and study. It must not be used for any other purposes and may not be transmitted or shared with others without prior permission.en_AU
usyd.facultySeS faculties schools::Faculty of Science::School of Physicsen_AU
usyd.degreeDoctor of Philosophy Ph.D.en_AU
usyd.awardinginstThe University of Sydneyen_AU
usyd.advisorLeon-Saval, Sergio
usyd.include.pubYesen_AU


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