Tytuł artykułu
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Wybrane pełne teksty z tego czasopisma
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Języki publikacji
Abstrakty
We present the results of our search for nearby planetary companions of transiting hot Jupiters in 12 planetary systems: HAT-P-24, HAT-P-39, HAT-P-42, HAT-P-50, KELT-2, KELT-15, KELT-17, WASP-23, WASP-63, WASP-76, WASP-79, and WASP-161. Our analysis was based on multi-sector time-series photometry from the Transiting Exoplanet Survey Satellite and precise transit timing data sets. We detected no additional transiting planets down to the 2-4 Earth radii regime. For ten hot Jupiters, no departure from linear transit ephemerides was observed. Whilst we refute long-term variations of the orbital period for WASP-161 b, which were claimed in the literature, we notice a tentative hint of the orbital period shortening for WASP-79 b. In addition, we spot a short-period transit timing variation for KELT-2A b with the characteristics typical of the so-called exomoon corridor. We conclude, however, that further observations are required to confirm these findings.
Słowa kluczowe
stars: individual: HAT-P-24
stars: individual: HAT-P-39
stars: individual: HAT-P-42
stars: individual: HAT-P-5
stars: individual: KELT-2
stars: individual: KELT-15
stars: individual: KELT-17
stars: individual: WASP-23
stars: individual: WASP-6
stars: individual: WASP-76
stars: individual: WASP-79
stars: individual: WASP-161
planets and satellites: individual: HAT-P-24 b
planets and satellites: individual: HAT-P-39 b
planets and satellites: individual: HAT-P-42 b
planets and satellites: individual: HAT-P-50 b
planets and satellites: individual: KELT-2 b
planets and satellites: individual: KELT-15 b
planets and satellites: individual: KELT-17 b
planets and satellites: individual: WASP-23 b
planets and satellites: individual: WASP-63 b
planets and satellites: individual: WASP-76 b
planets and satellites: individual: WASP-79 b
planets and satellites: individual: WASP-161 b
Czasopismo
Rocznik
Tom
Strony
159--177
Opis fizyczny
Bibliogr. 70 poz., tab., wykr.
Twórcy
autor
- Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziądzka 5, 87-100 Toruń, Poland
autor
- Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziądzka 5, 87-100 Toruń, Poland
autor
- Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziądzka 5, 87-100 Toruń, Poland
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Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-4401b82d-3633-4807-8e64-aee5cda971f2