2024
Validation of selected TESS exoplanetary candidates
MESARČ, Marko a Ľubomír HAMBÁLEKZákladní údaje
Originální název
Validation of selected TESS exoplanetary candidates
Autoři
MESARČ, Marko (703 Slovensko, domácí) a Ľubomír HAMBÁLEK (703 Slovensko)
Vydání
Contributions of the Astronomical Observatory Skalnaté Pleso, Astronomical Institute, Slovak Academy of Sciences, 2024, 1335-1842
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Slovensko
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 0.500 v roce 2022
Organizační jednotka
Přírodovědecká fakulta
UT WoS
001178776600007
Klíčová slova anglicky
Planetary systems; Binaries: eclipsing; Techniques: photometric
Štítky
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 9. 4. 2024 14:52, Mgr. Marie Šípková, DiS.
Anotace
V originále
We have selected suitable 6 exoplanetary candidates from the TESS database which were observable using a network of small ground-based telescopes to collect photometric transits during follow-up observation. We have made a new reduction of TESS photometry using a custom aperture, as well as reducing the ground-based aperture photometry. We have refined the period of transits and constructed O - C diagrams. Mean transit was fitted in all observed photometric filters and we derived individual candidate's physical parameters. Using the colour indices during transit, we hint at the exoplanetary nature of candidates. Three targets TOI-1518b, TOI-2046b, and TOI-2109b were confirmed as exoplanets by other authors during the writing of this thesis. Here, we have provided an independent evaluation and analysis, without any knowledge of their results. TOI-3856.01 is among the targets more likely a substellar object based on my results, but it has not been confirmed yet. In the case of TOI-1834.01, we have proposed another scenario incompatible with the original assumption that it was an exoplanetary candidate and we assume that it is a hierarchical triple system. TOI-3604.01 was also modelled concerning parasitic light in the aperture. Individual models suggest a body too large for an exoplanet.