Mock HI spectral line stacking experiments for large galaxy surveys

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dc.contributor.advisorElson, Ed
dc.contributor.advisorMaartens, Roy
dc.contributor.authorTladi, Modisha
dc.date.accessioned2020-11-03T07:34:20Z
dc.date.accessioned2024-10-30T10:24:01Z
dc.date.available2020-11-03T07:34:20Z
dc.date.available2024-10-30T10:24:01Z
dc.date.issued2019
dc.description>Magister Scientiae - MScen_US
dc.description.abstractThe study of neutral atomic hydrogen (HI) plays a vital role in improving the knowledge about galaxy evolution since HI serves as the raw fuel for star formation. However, the current knowledge about it is limited to the nearby Universe due to its intrinsic faintness and the inadequate sensitivities of the current radio telescopes.en_US
dc.identifier.urihttps://hdl.handle.net/10566/16707
dc.language.isoenen_US
dc.publisherUniversity of Western Capeen_US
dc.rights.holderUniversity of Western Capeen_US
dc.subjectNeutral atomic hydrogenen_US
dc.subjectAstronomyen_US
dc.subjectCASA (Common Astronomy Software Applications).en_US
dc.subjectGalaxyen_US
dc.titleMock HI spectral line stacking experiments for large galaxy surveysen_US

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