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dc.contributor.authorTremblay, Chenoa
dc.contributor.supervisorSteven Tingayen_US
dc.date.accessioned2018-12-19T00:13:59Z
dc.date.available2018-12-19T00:13:59Z
dc.date.issued2018
dc.identifier.urihttp://hdl.handle.net/20.500.11937/70728
dc.description.abstract

I used a wide-field, low-frequency telescope to search for signals from molecules, atoms, and exo-planets, surveying the Galactic Centre and Orion to detect molecules for the first time below 700MHz. In collaboration, I used the same data to set upper limits on the signal strength of extraterrestrial civilisations. Utilising surveys at infrared and radio wavelengths, I found evidence that high-mass stars can form in isolation.

en_US
dc.publisherCurtin Universityen_US
dc.titleA Search for Molecules at Low Frequency with the Murchison Widefield Arrayen_US
dc.typeThesisen_US
dcterms.educationLevelPhDen_US
curtin.departmentElectrical Engineering, Computer and Math Science (EECMS)en_US
curtin.accessStatusOpen accessen_US
curtin.facultyScience and Engineeringen_US


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