The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle: The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability.

Aaron Golden

The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle: The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability.

Physics

Research output: Contribution to conference (Published) › Poster

Original language	English (Ireland)
Publication status	Published - 1 Jan 2021
Event	The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. 2021 - Duration: 2 Mar 2021 → …

Conference

Conference	The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. 2021
Period	2/03/21 → …

Authors (Note for portal: view the doc link for the full list of authors)

Authors
Dulaimi, Salam; Fitzgerald, Karol; Boyle, Richard P.; Golden, Aaron; Butler, Ray F.

Cite this

Golden, A. (2021). The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle: The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability. . Poster session presented at The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. 2021.

Golden, Aaron. / The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle : The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability. . Poster session presented at The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. 2021.

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title = "The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle: The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability. ",

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year = "2021",

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Golden, A 2021, 'The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle: The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability. ', The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. 2021, 2/03/21.

The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle: The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability. . / Golden, Aaron.
2021. Poster session presented at The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. 2021.

Research output: Contribution to conference (Published) › Poster

Golden A. The Light Curve Fitter: A novel application for deconvolving two superimposed sinusoidal waves developed using the Agile Software Development Lifecycle: The Galway Ultra-Fast Imager (GUFI) located on the 1.8m Vatican Advanced Technology Telescope (VATT) was tasked to monitor tight brown dwarf binaries. However, due to the close separation between the components in these binaries, the GUFI photometer could not image each component of binary systems as a point source in our campaign. Therefore, we developed and employed our novel application, the Light Curve Fitter, which is capable of distinguishing two superimposed sinusoidal waves. This application allows users to untangle the secondary components variability signature from that of the dominant primary variability. . 2021. Poster session presented at The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. 2021.