Search for Planets in Hot Jupiter Systems with Multi-Sector TESS Photometry. II. Constraints on Planetary Companions in 12 Systems

• Autorzy: Maciejewski G.

Identyfikatory

DOI

10.32023/0001-5237/72.1.1

• Języki publikacji: EN

Abstrakty

EN

Uninterrupted observations from space-borne telescopes provide the photometric precision that is required to detect shallow transits of small planets missed by ground-based surveys. We used data from the Transiting Exoplanet Survey Satellite (TESS) to search for nearby planetary companions in 12 planetary systems with hot Jupiters: HD 2685, Qatar-10, WASP-4, WASP-48, WASP-58, WASP-91, WASP-120, WASP-121, WASP-122, WASP-140, XO-6, and XO-7. We also applied the transit timing method based on homogeneously determined mid-transit times in order to search for non-transiting companions that could gravitationally perturb the already known planets. We found no additional planets in those systems down to the regime of sub-Neptunian globes. This negative result is in line with statistical studies, supporting the high-eccentricity migration as a pathway of the investigated giant planets to the tight orbits observed today.

Słowa kluczowe

EN

Stars: individual: HD 2685; Stars: individual: Qatar-10; Stars: individual: WASP-4; Stars: individual: WASP-48; Stars: individual: WASP-58; Stars: individual: WASP-91; Stars: individual: WASP-120; Stars: individual: WASP-121; Stars: individual: WASP-122; Stars: individual: WASP-140; Stars: individual: XO-6; Stars: individual: XO-7; Planets and satellites: individual: HD 2685 b; Planets and satellites: individual Qatar-10 b; Planets and satellites: individual WASP-4 b; Planets and satellites: individual WASP-48 b; Planets and satellites: individual WASP-58 b; Planets and satellites: individual WASP-91 b; Planets and satellites: individual WASP-120 b; Planets and satellites: individual WASP-121 b; Planets and satellites: individual WASP-122 b; Planets and satellites: individual WASP-140 b; Planets and satellites: individual XO-6 b; Planets and satellites: individual XO-7 b

• Wydawca: Copernicus Foundation for Polish Astronomy
• Czasopismo: Acta Astronomica
• Rocznik: 2022
• Tom: Vol. 72, No. 1
• Strony: 1--19
• Opis fizyczny: Bibliogr. 69 poz., tab., wykr.

Twórcy

autor

Maciejewski G.

• Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Grudziadzka 5, 87-100 Toruń, Poland

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Uwagi

Opracowanie rekordu ze środków MEiN, umowa nr SONP/SP/546092/2022 w ramach programu "Społeczna odpowiedzialność nauki" - moduł: Popularyzacja nauki i promocja sportu (2022-2023)