Mock HI spectral line stacking experiments for large galaxy surveys

dc.contributor.advisor	Elson, Ed
dc.contributor.advisor	Maartens, Roy
dc.contributor.author	Tladi, Modisha
dc.date.accessioned	2020-11-03T07:34:20Z
dc.date.available	2020-11-03T07:34:20Z
dc.date.issued	2019
dc.identifier.uri	http://hdl.handle.net/11394/7413
dc.description	>Magister Scientiae - MSc	en_US
dc.description.abstract	The 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.language.iso	en	en_US
dc.publisher	University of Western Cape	en_US
dc.subject	Neutral atomic hydrogen	en_US
dc.subject	Astronomy	en_US
dc.subject	CASA (Common Astronomy Software Applications).	en_US
dc.subject	Galaxy	en_US
dc.title	Mock HI spectral line stacking experiments for large galaxy surveys	en_US
dc.rights.holder	University of Western Cape	en_US