The near infrared luminosity function of the Norma Cluster

dc.contributor.advisorKraan-Korteweg, Renee
dc.contributor.advisorWoudt, Patrick
dc.contributor.authorSkelton, R.E
dc.date.accessioned2024-06-19T09:21:23Z
dc.date.available2024-06-19T09:21:23Z
dc.date.issued2007
dc.date.updated2024-06-19T09:09:31Z
dc.description.abstractIn this thesis, a near infrared KB-band photometric catalogue of galaxies in the Nonna cluster is presented. The survey of the cluster covers an area of '" 0.8h702 Mpc2, and is estimated to be complete to a magnitude of MK. ⋨-19 mag; this extends into the dwarf regime, 6 magnitudes below M'k •. The catalogue contains 390 objects, 235 of which are classified as likely or definite galaxies and 155 as candidate galaxies. The K.,-band luminosity function (LF) is constructed from the photometric sample, using a smaller spectroscopic survey to estimate the number of member galaxies at each magnitude. A Schechter function provides a reasonable fit to the data, with a characteristic magnitude of M'k. = -25.36 ± 0.74 mag and faint-end slope of a = -1.25 ± 0.10. There is a distinct dip in the LF at MK. '" -22 mag. The shape of the LF is similar to those found in previous determinations of the cluster LF, in both optical and near infrared. The Schechter parameters obtained by flagging the dip point agree well with those of recent field LFs. This suggests that both the shape of the bright end and the faint end slope are relatively insensitive to environment.
dc.identifier.apacitationSkelton, R. E. (2007). <i>The near infrared luminosity function of the Norma Cluster</i>. (). ,Faculty of Science ,Department of Astronomy. Retrieved from http://hdl.handle.net/11427/39967en_ZA
dc.identifier.chicagocitationSkelton, R.E. <i>"The near infrared luminosity function of the Norma Cluster."</i> ., ,Faculty of Science ,Department of Astronomy, 2007. http://hdl.handle.net/11427/39967en_ZA
dc.identifier.citationSkelton, R.E. 2007. The near infrared luminosity function of the Norma Cluster. . ,Faculty of Science ,Department of Astronomy. http://hdl.handle.net/11427/39967en_ZA
dc.identifier.ris TY - Thesis / Dissertation AU - Skelton, R.E AB - In this thesis, a near infrared KB-band photometric catalogue of galaxies in the Nonna cluster is presented. The survey of the cluster covers an area of '" 0.8h702 Mpc2, and is estimated to be complete to a magnitude of MK. ⋨-19 mag; this extends into the dwarf regime, 6 magnitudes below M'k •. The catalogue contains 390 objects, 235 of which are classified as likely or definite galaxies and 155 as candidate galaxies. The K.,-band luminosity function (LF) is constructed from the photometric sample, using a smaller spectroscopic survey to estimate the number of member galaxies at each magnitude. A Schechter function provides a reasonable fit to the data, with a characteristic magnitude of M'k. = -25.36 ± 0.74 mag and faint-end slope of a = -1.25 ± 0.10. There is a distinct dip in the LF at MK. '" -22 mag. The shape of the LF is similar to those found in previous determinations of the cluster LF, in both optical and near infrared. The Schechter parameters obtained by flagging the dip point agree well with those of recent field LFs. This suggests that both the shape of the bright end and the faint end slope are relatively insensitive to environment. DA - 2007 DB - OpenUCT DP - University of Cape Town KW - Astronomy LK - https://open.uct.ac.za PY - 2007 T1 - The near infrared luminosity function of the Norma Cluster TI - The near infrared luminosity function of the Norma Cluster UR - http://hdl.handle.net/11427/39967 ER - en_ZA
dc.identifier.urihttp://hdl.handle.net/11427/39967
dc.identifier.vancouvercitationSkelton RE. The near infrared luminosity function of the Norma Cluster. []. ,Faculty of Science ,Department of Astronomy, 2007 [cited yyyy month dd]. Available from: http://hdl.handle.net/11427/39967en_ZA
dc.language.rfc3066eng
dc.publisher.departmentDepartment of Astronomy
dc.publisher.facultyFaculty of Science
dc.subjectAstronomy
dc.titleThe near infrared luminosity function of the Norma Cluster
dc.typeThesis / Dissertation
dc.type.qualificationlevelMasters
dc.type.qualificationlevelMasters
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