A new approach to classical spectroscopy
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Type
ThesisThesis type
Doctor of PhilosophyAuthor/s
Betters, Christopher HaroldAbstract
In this thesis I demonstrate a new approach to classical fibre-fed spectroscopy. My method is to use a photonic lantern device that converts an arbitrary (e.g. incoherent) input beam into N diffraction-limited outputs. For the highest throughput, the number of outputs must be ...
See moreIn this thesis I demonstrate a new approach to classical fibre-fed spectroscopy. My method is to use a photonic lantern device that converts an arbitrary (e.g. incoherent) input beam into N diffraction-limited outputs. For the highest throughput, the number of outputs must be matched to the total number of unpolarised spatial modes on input. This approach has many advantages: (i) after the lantern, the instrument is constructed from ‘commercial off the shelf’ components; (ii) the instrument is the minimum size and mass configuration at a fixed resolving power and spectral order; (iii) the throughput can be better than 60% (slit to detector, including detector QE of ~80%); (iv) the scattered light at the detector can be less than 0.1% (total power). I have designed and built 3 such instruments, one operating in the infrared and two operating in the visible wavelengths of light. What follows is a study of the design implications for such a spectrograph, and an experimental exploration of their characteristics. I also present a versatile data reduction package I have developed in tandem with the instruments.
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See moreIn this thesis I demonstrate a new approach to classical fibre-fed spectroscopy. My method is to use a photonic lantern device that converts an arbitrary (e.g. incoherent) input beam into N diffraction-limited outputs. For the highest throughput, the number of outputs must be matched to the total number of unpolarised spatial modes on input. This approach has many advantages: (i) after the lantern, the instrument is constructed from ‘commercial off the shelf’ components; (ii) the instrument is the minimum size and mass configuration at a fixed resolving power and spectral order; (iii) the throughput can be better than 60% (slit to detector, including detector QE of ~80%); (iv) the scattered light at the detector can be less than 0.1% (total power). I have designed and built 3 such instruments, one operating in the infrared and two operating in the visible wavelengths of light. What follows is a study of the design implications for such a spectrograph, and an experimental exploration of their characteristics. I also present a versatile data reduction package I have developed in tandem with the instruments.
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Date
2015-04-01Licence
The 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.Faculty/School
Faculty of Science, School of PhysicsAwarding institution
The University of SydneyShare