Show simple item record

Blazar Microvariations

dc.contributor.advisorProfessor Robert Knop
dc.contributor.authorPittman, Cameron W.
dc.date.accessioned2009-05-07T15:33:26Z
dc.date.available2009-05-07T15:33:26Z
dc.date.issued2009-04-20
dc.identifier.urihttp://hdl.handle.net/1803/2944
dc.descriptionHonors in Astronomy
dc.description.abstractIn November 2006, the authors collected data on blazars PKS 0537-441, PKS 0447-439, and PKS 0208-5121 from the Cerra Tololo Inter-American Observatory in Chile. All three blazars are tested for microvariability, first by comparing relative magnitudes against unvarying stars, then through power spectrum analysis. The authors used GNU Scientific Library tools for the Fourier transforms needed for power spectrum analysis. Fourier transforms break down data into series of periodic functions. Running power spectra quantitatively illuminate periodicity and variability in data. The authors tested power spectra by using well-defined functions to better understand power spectra analysis. Through light curve analysis and power spectra analysis, the authors found PKS 0537-441 showed microvariability, PKS 0208-512 most likely did not show microvariability, and PKS 0447-439 did not show microvariability.en
dc.language.isoen_USen
dc.publisherVanderbilt University. Dept. of Physics and Astronomyen
dc.subjectBlazaren
dc.subjectPKS 0537-441en
dc.subjectPKS 0447-439en
dc.subjectPKS 0208-512en
dc.subjectMicrovariabilityen
dc.subjectMicrovariationsen
dc.subjectPower spectraen
dc.subjectQuasaren
dc.subjectBlazarsen
dc.subject.lcshBL Lacertae objectsen
dc.subject.lcshFourier transformationsen
dc.subject.lcshPower spectraen
dc.subject.lcshLight curvesen
dc.subject.lcshQuasarsen
dc.titleBlazar Microvariationsen
dc.typeThesisen
dc.description.collegeCollege of Arts and Scienceen
dc.description.schoolVanderbilt Universityen
dc.description.departmentDepartment of Physics and Astronomyen


Files in this item

Icon

This item appears in the following Collection(s)

Show simple item record