2026-09-19T16:26:09.437454800Zhttps://opus.uleth.ca/server/oai/requestoai:opus.uleth.ca:10133/2912015-11-04T19:42:33Zcom_10133_3346com_10133_1com_10133_296col_10133_3347col_10133_298
ULethbridge OPUS Repository
supervisor
Naylor, David A.
author
Spencer, Locke Dean
author
University of Lethbridge. Faculty of Arts and Science
2007-05-23T20:46:01Z
2007-05-23T20:46:01Z
2005
https://hdl.handle.net/10133/291
The European Space Agency's Herschel Space Observatory is comprised of three cryogenically cooled instruments commissioned to explore the far infrared/submillimetre universe. The Spectral and Photometric Imaging REceiver (SPIRE) is one of Herschel's instruments and consists of a three band imaging photometer and a two band imaging spectrometer. Canada is involved in the SPIRE project through provision of instrument development hardware and software, mission flight software, and support personnel. This thesis discusses Fourier transform spectroscopy (FTS) and FTS data processing. A detailed discussion is included on FTS phase correction, with results presented from the optimization of an enhanced Forman phase correction routine developed for this work. This thesis discusses the design, verification, and use of the hardware and software provided by Dr. Naylor's group as it relates to SPIRE verification testing. Results of the photometer characterization are presented. The current status of SPIRE and its future schedule is also discussed.
en_US
Dissertations, Academic
Astronomical photometry
Infrared astronomy
Fourier transform spectroscopy
Spectral and Photometric Imaging REceiver (SPIRE)
Spectral characterization of the Herschel SPIRE photometer
Thesis
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URL
http://localhost:4000/bitstreams/9c8433dc-8ffc-4e3a-a673-9139ecd7a93d/download
File
MD5
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application/pdf
MR17424.pdf
URL
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File
MD5
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MR17424.pdf.txt