A dataset provided by the European Space Agency

Obs ID 2298637
Target/Line-of-sight Escape from the V1298 Tau e labyrinth: following the CHEOPS thread to confirm the orbital period and large TTVs/TDVs of an infant planet
Gaia DR2 ID Gaia DR2 51886335968692480
URL https://cheops.unige.ch/archive_browser/?visit-id=2298637
DOI https://doi.org/10.57780/esa-l241kl8
Author European Space Agency, Mario damasso
Description of observation
  • Target RA (J2000): 61.3316307067871 °
  • Target Dec (J2000): 20.1571006774902 °
  • Gaia GMag: 10.08
  • Programme ID: CH_PR240005
  • PI of observing programme: Mario damasso
  • Title of programme: Escape from the V1298 Tau e labyrinth: following the CHEOPS thread to confirm the orbital period and large TTVs/TDVs of an infant planet
  • Abstract: The object of the proposal is the star V1298 Tau, which hosts a system of four transiting planets. The focus of the science case is the confirmation of the orbital period of planet V1298 Tau e, and the determination of its transit timing variations (TTVs) and transit duration variations (TDVs) also using archival photometric data collected by Kepler/K2 in 2015, and by TESS in 2021. Previous observations with CHEOPS allowed to identify P=45.00 days as the actual orbital period of planet e (private communication). This results must be necessarily confirmed with further follow-up, aimed at detecting additional transits. The same CHEOPS observations revealed a significant TTV and TDV. Observing new transits with CHEOPS is the only way to measure the average orbital period and the TTVs/TDVs, and to inform dynamical simulations in order to characterise the evolution of the planets orbits over very short timescale (of the order of a few years). The outstanding results expected from the follow-up with CHEOPS will be of great benefit for a proper modelling of hundreds of radial velocities of V1298 Tau collected so far, whose analysis has proved very challenging so far.
Temporal Coverage 2023-12-11T03:59:54Z / 2023-12-13T23:39:00Z
Version 3.0
Mission Description CHEOPS (Benz et al., https://doi.org/10.1007/s10686-020-09679-4) is a European Space Agency (ESA) mission in partnership with Switzerland with important contributions to the payload and the ground segment from Austria, Belgium, France, Germany, Hungary, Italy, Portugal, Spain, Sweden and the United Kingdom.

The satellite has a single payload comprising an ultra-high precision photometer covering the 330 - 1100 nm wavelength range in a single photometric band. Observations are made as part of the Guaranteed Time Observing Programme that is formulated by the CHEOPS Science Team, and the Guest Observers Programme through which the Community at large can apply for CHEOPS time.
Creator Contact https://www.cosmos.esa.int/web/cheops/contact
Date Published 2025-10-01T12:39:23Z
Keywords CHEOPS, EXOPLANETS, wide-band photometer
Acknowledgements https://www.cosmos.esa.int/web/cheops-guest-observers-programme/publication-guidelines
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Mario damasso et al., 2025, 'Escape from the "V1298 Tau e labyrinth": following the CHEOPS' thread to confirm the orbital period and large TTVs/TDVs of an infant planet', 3.0, European Space Agency, https://doi.org/10.57780/esa-l241kl8