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dc.contributor.advisorKantowski, Ronald,en_US
dc.contributor.authorBagherpour, Hamed.en_US
dc.date.accessioned2013-08-16T12:20:20Z
dc.date.available2013-08-16T12:20:20Z
dc.date.issued2006en_US
dc.identifier.urihttps://hdl.handle.net/11244/1074
dc.description.abstractIn this dissertation we concentrate on some of these effects on the observation of type Ia supernovae.en_US
dc.description.abstractGravitational lensing has turned out to be an active field in astronomy, both as an abstract subject and a means to better understand and study other astronomical topics. One of the main applications of gravitational lensing is the broad field of supernovae observation. It is shown that lensing can have dramatic effects on how supernovae are observed, and therefore appear as an inevitable 'noise' in any (deep) survey carried out for purposes such as determining the equation of state for the so-called dark energy.en_US
dc.format.extentxiii, 88 leaves :en_US
dc.subjectPhysics, Astronomy and Astrophysics.en_US
dc.subjectMicrolensing (Astrophysics)en_US
dc.subjectSupernovae.en_US
dc.titleOn the gravitational lensing of type Ia supernovae.en_US
dc.typeThesisen_US
dc.thesis.degreePh.D.en_US
dc.thesis.degreeDisciplineHomer L. Dodge Department of Physics and Astronomyen_US
dc.noteSource: Dissertation Abstracts International, Volume: 67-06, Section: B, page: 3177.en_US
dc.noteAdviser: Ronald Kantowski.en_US
ou.identifier(UMI)AAI3222153en_US
ou.groupCollege of Arts and Sciences::Homer L. Dodge Department of Physics and Astronomy


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