Publication: Ground-Based Follow-Up Observations of TESS Object of Interest TOI 3779.1
| dc.contributor.advisor | Plavchan, Peter | |
| dc.contributor.author | Olaiz, Estefanía | |
| dc.date.accessioned | 2024-04-17T18:07:29Z | |
| dc.date.available | 2024-04-17T18:07:29Z | |
| dc.date.issued | 2023-10 | |
| dc.description.abstract | This study presents the identification of an eclipsing binary system consisting of a 1.618-day orbital period, as determined through follow-up observations of the TESS Object of Interest (TOI) 3779.01 (TIC 275527293). Leveraging data from the Transiting Exoplanet Survey Satellite (TESS) and ground-based observations from George Mason University's 16″ Dobsonian Strickland telescope in Fairfax, VA, Multi-Aperture Photometry using AstroImageJ (AIJ) was performed for photometric measurements, light curve plotting, and transit analysis. The resulting light curve and validation tests suggest TOI-3779.1 is likely an eclipsing binary system. All outcomes, including light curves, detrended data, and measurements, were submitted to ExoFOP (Exoplanet Follow-up Observation Program) for further examination and archiving. | |
| dc.identifier.uri | http://hdl.handle.net/1920/13600 | |
| dc.identifier.uri | https://doi.org/10.13021/MARS/2060 | |
| dc.language.iso | en | |
| dc.publisher | George Mason University | |
| dc.rights | Copyright 2023 Estefanía Olaiz | |
| dc.rights.uri | https://rightsstatements.org/page/InC/1.0/ | |
| dc.title | Ground-Based Follow-Up Observations of TESS Object of Interest TOI 3779.1 | |
| dc.type | Project | |
| dspace.entity.type | Publication |