A search for transit timing variations in the HATS-18 planetary system

John Southworth*, A. J. Barker, T. C. Hinse, Y. Jongen, M. Dominik, U. G. Jørgensen, P. Longa-Peña, S. Sajadian, C. Snodgrass, J. Tregloan-Reed, N. Bach-Møller, M. Bonavita, V. Bozza, M. J. Burgdorf, R. Figuera Jaimes, Ch Helling, J. A. Hitchcock, M. Hundertmark, E. Khalouei, H. KorhonenL. Mancini, N. Peixinho, S. Rahvar, M. Rabus, J. Skottfelt, P. Spyratos

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract / Description of output

HATS-18 b is a transiting planet with a large mass and a short orbital period, and is one of the best candidates for the detection of orbital decay induced by tidal effects. We present extensive photometry of HATS-18 from which we measure 27 times of mid-transit. Two further transit times were measured from data from the Transiting Exoplanet Survey Satellite (TESS) and three more taken from the literature. The transit timings were fitted with linear and quadratic ephemerides and an upper limit on orbital decay was determined. This corresponds to a lower limit on the modified stellar tidal quality factor of Q′⋆>105.11±0.04⁠. This is at the cusp of constraining the presence of enhanced tidal dissipation due to internal gravity waves. We also refine the measured physical properties of the HATS-18 system, place upper limits on the masses of third bodies, and compare the relative performance of TESS and the 1.54 m Danish Telescope in measuring transit times for this system.
Original languageEnglish
Pages (from-to)3212-3223
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Issue number3
Early online date12 Jul 2022
Publication statusPublished - 1 Sept 2022

Keywords / Materials (for Non-textual outputs)

  • planetary systems
  • stars: fundamental parameters
  • stars: individual: HATS-18


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