Introducing PHOEBE: An Eclipsing Companion Modeling Software Package

dc.contributor.authorLevsey, Dylan
dc.date.accessioned2021-08-09T13:54:50Z
dc.date.available2021-08-09T13:54:50Z
dc.date.created2020
dc.description2020 Student Celebration of Research and Creativity presentationen_US
dc.description.abstractOne of the primary ways that we can detect stellar companions is by looking for transits. A transit is when the companion passes in front of or behind its host star. In this poster, we will introduce the Python package PHOEBE as well as present the different visualizations of the model that PHOEBE is capable of creating for a given transiting system. Our model can be visualized in four different ways: mesh model, photometric lightcurve, radial velocity curve, and astrometric orbit. We will ultimately use this package to analyze data from the APOGEE and TESS surveys.en_US
dc.description.urihttps://youtu.be/b5dAh-Etpj8en_US
dc.identifier.urihttp://hdl.handle.net/11216/3872
dc.language.isoen_USen_US
dc.publisherNorthern Kentucky Universityen_US
dc.relation.ispartofseriesCelebration of Student Research and Creativity;2020
dc.subjectPython (Computer program language)en_US
dc.subjectStarsen_US
dc.subjectTransit-instrumentsen_US
dc.titleIntroducing PHOEBE: An Eclipsing Companion Modeling Software Packageen_US
dc.typePresentationen_US

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