A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work

 

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dc.contributor.advisor Kraan-Korteweg, Renée C en_ZA
dc.contributor.advisor Jarrett, Thomas en_ZA
dc.contributor.author Affadi, Ikechukwu Patrick en_ZA
dc.date.accessioned 2016-07-26T12:22:42Z
dc.date.available 2016-07-26T12:22:42Z
dc.date.issued 2016 en_ZA
dc.identifier.citation Affadi, I. 2016. A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work. University of Cape Town. en_ZA
dc.identifier.uri http://hdl.handle.net/11427/20813
dc.description.abstract This thesis aims at using the Infrared Survey Facility (IRSF) JHKₛ bands, Two Micron All Sky Survey (2MASS) JHKₛ bands and Wide Field Infrared Survey Explorer (WISE) W1-W4 bands isophotal magnitudes to understand the cosmic flow associated with Zone of Avoidance (ZoA) galaxies. en_ZA
dc.language.iso eng en_ZA
dc.subject.other Astronomy en_ZA
dc.subject.other Astrophysics and Space Science en_ZA
dc.title A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work en_ZA
dc.type Master Thesis
uct.type.publication Research en_ZA
uct.type.resource Thesis en_ZA
dc.publisher.institution University of Cape Town
dc.publisher.faculty Faculty of Science en_ZA
dc.publisher.department Department of Astronomy en_ZA
dc.type.qualificationlevel Masters
dc.type.qualificationname MSc en_ZA
uct.type.filetype Text
uct.type.filetype Image
dc.identifier.apacitation Affadi, I. P. (2016). <i>A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work</i>. (Thesis). University of Cape Town ,Faculty of Science ,Department of Astronomy. Retrieved from http://hdl.handle.net/11427/20813 en_ZA
dc.identifier.chicagocitation Affadi, Ikechukwu Patrick. <i>"A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work."</i> Thesis., University of Cape Town ,Faculty of Science ,Department of Astronomy, 2016. http://hdl.handle.net/11427/20813 en_ZA
dc.identifier.vancouvercitation Affadi IP. A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work. [Thesis]. University of Cape Town ,Faculty of Science ,Department of Astronomy, 2016 [cited yyyy month dd]. Available from: http://hdl.handle.net/11427/20813 en_ZA
dc.identifier.ris TY - Thesis / Dissertation AU - Affadi, Ikechukwu Patrick AB - This thesis aims at using the Infrared Survey Facility (IRSF) JHKₛ bands, Two Micron All Sky Survey (2MASS) JHKₛ bands and Wide Field Infrared Survey Explorer (WISE) W1-W4 bands isophotal magnitudes to understand the cosmic flow associated with Zone of Avoidance (ZoA) galaxies. DA - 2016 DB - OpenUCT DP - University of Cape Town LK - https://open.uct.ac.za PB - University of Cape Town PY - 2016 T1 - A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work TI - A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work UR - http://hdl.handle.net/11427/20813 ER - en_ZA


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