Developing an Open Source Predictive Spot Model for Use in Brown Dwarf Photometry

Author(s)Dettman, Kyle
Date Accessioned2015-10-07T17:46:11Z
Date Available2015-10-07T17:46:11Z
Publication Date2015-05
AbstractWhen studying ultracool stars such as brown dwarfs some of the most infor- mative data comes photometric observations. These observations, though limited in its accuracy due to the limitations of the collector, provide insight into features of the atmosphere that produce uctuations in the light curve. It is commonly thought that the uctuations are caused by traditional spots in the star's atmosphere, though analyzing the data can be di cult due to the sometimes sporadic data. This paper seeks to create an open source program which can analyze this photometric data and provide suggestions as to the structure of the spot to produce such a curve. It will also look at the typical features of spots and determine if the features that are seen on these stars are actually consistent with these features or if it some new phenomena such as clouds or other weather related structures.
AdvisorJohn Gizis
ProgramPhysics and Astronomy
URLhttp://udspace.udel.edu/handle/19716/17071
Languageen_USen_US
PublisherUniversity of Delawareen_US
KeywordsPhysicsen_US
KeywordsResearch Subject Categories::NATURAL SCIENCES::Physics::Astronomy and astrophysics::Astronomyen_US
TitleDeveloping an Open Source Predictive Spot Model for Use in Brown Dwarf Photometryen_US
TypeThesisen_US
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