The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
arXiv:2604.15035 · doi:10.1051/0004-6361/202558740
Abstract
Following the 2022 alert of a TESS object of interest transiting TOI-5624 (a G7 V star 100 pc away), a CHEOPS campaign in 2023 detected four planetary signals at , , , and days, later confirmed by additional TESS and CHEOPS photometry in 2024-2025. After analysing the TESS & CHEOPS photometric data, we extracted and modelled the HARPS-N & SOPHIE RV time series using two independent methodologies both within an MCMC framework. We further integrated the N-body equations of motion, while simultaneously fitting the transit times and the detrended RVs, to dynamically characterise the system. We present the discovery of four transiting sub-Neptunes with radii of , , , and and masses of , , , and . Our photometric analysis reveals that the outermost transiting planet TOI-5624 e shows significant TTVs. We find a robust Keplerian signal in the RV time series close to the 2:1 period commensurability with TOI-5624 e, which explains the TTV pattern exhibited by TOI-5624 e according to our dynamical analysis. We label this non-transiting planet as TOI-5624 f and find its minimum mass to be . Among the known systems hosting more than four planets, the remarkable precision with which the radii have been measured (<1.7%) and the firm assessment (>3) of the mass for at least three planets has been previously reached only for TRAPPIST-1. Additional photometric observations will enable a better sample of the TTV modulation and a more robust dynamical determination of the masses.
Accepted for publication in A&A. 22 pages (13 in the main text), 4 figures (+9 in the Appendix), 2 tables (+7 in the Appendix). Abstract abridged to satisfy the arXiv submission requirements
References in corpus (75)
- emcee: The MCMC Hammer
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- Gaia Data Release 3: Summary of the content and survey properties
- The Transiting Exoplanet Survey Satellite
- The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms
- A new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase
- Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction
- Fast and scalable Gaussian process modeling with applications to astronomical time series
- Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position
- DHP Framework: Digital Health Passports Using Blockchain -- Use case on international tourism during the COVID-19 pandemic
- On detecting terrestrial planets with timing of giant planet transits
- Kepler Presearch Data Conditioning I - Architecture and Algorithms for Error Correction in Kepler Light Curves
- Spectroscopic parameters for 451 stars in the HARPS GTO planet search program. Stellar [Fe/H] and the frequency of exo-Neptunes
- The CORALIE survey for southern extra-solar planets VII. Two short-period Saturnian companions to HD108147 and HD168746
- The effect of red noise on planetary transit detection
- The Transiting Exoplanet Survey Satellite: Simulations of planet detections and astrophysical false positives
- THE ORIGIN OF PLUTO'S ORBIT: IMPLICATIONS FOR THE SOLAR SYSTEM BEYOND NEPTUNE
- A Gaussian process framework for modelling stellar activity signals in radial velocity data
- The HARPS-TERRA project I. Description of the algorithms, performance and new measurements on a few remarkable stars observed by HARPS
- Extracting Planet Mass and Eccentricity From TTV data
- A new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)
- The California-Kepler Survey V. Peas in a Pod: Planets in a Kepler Multi-planet System are Similar in Size and Regularly Spaced
- A new list of thorium and argon spectral lines in the visible
- SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs I. New atmospheric parameters and masses for 48 stars with planets
- The CHEOPS mission
- Limb darkening and exoplanets: testing stellar model atmospheres and identifying biases in transit parameters
- CLES, Code Liegeois d'Evolution Stellaire
- Transit Least Squares: Optimized transit detection algorithm to search for periodic transits of small planets
- Kepler Planet Masses and Eccentricities from TTV Analysis
- ARES v2 - new features and improved performance
- Theoretical models of planetary system formation: mass vs semi-major axis
- Six transiting planets and a chain of Laplace resonances in TOI-178
- A pair of planets around HD 202206 or a circumbinary planet?
- Thermal emission at 4.5 and 8 micron of WASP-17b, an extremely large planet in a slightly eccentric orbit
- The HARPS search for southern extra-solar planets XIX. Characterization and dynamics of the GJ876 planetary system
- SOPHIE+: First results of an octagonal-section fiber for high-precision radial velocity measurements
- Planet formation models: the interplay with the planetesimal disc
- Expected performances of the Characterising Exoplanet Satellite (CHEOPS) III. Data reduction pipeline: architecture and simulated performances
- Age consistency between exoplanet hosts and field stars
- The SOPHIE search for northern extrasolar planets III. A Jupiter-mass companion around HD 109246
- Revising the ages of planet-hosting stars
- How planetary growth outperforms migration
- SWEET-Cat 2.0: The Cat just got SWEETer; Higher quality spectra and precise parallaxes from GAIA eDR3
- Measurement of planet masses with transit timing variations due to synodic "chopping" effects
- Pyaneti: a fast and powerful software suite for multi-planet radial velocity and transit fitting
- RUN DMC: An efficient, parallel code for analyzing Radial Velocity Observations using N-body Integrations and Differential Evolution Markov chain Monte Carlo
- pyaneti II: A multidimensional Gaussian process approach to analysing spectroscopic time-series
- Transiting planets - lightcurve analysis for eccentric orbits
- CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii
- Transit timing to first order in eccentricity
- A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS) -- I. Search for exoplanets and variable stars in the field of 47 Tuc
- TRADES: A new software to derive orbital parameters from observed transit times and radial velocities. Revisiting Kepler-11 and Kepler-9
- WASP-186 and WASP-187: two hot Jupiters discovered by SuperWASP and SOPHIE with additional observations by TESS
- A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067
- Enhanced constraints on the interior composition and structure of terrestrial exoplanets
- Reinvestigating Cen AB in light of asteroseismic forward and inverse methods
- HARPS-N radial velocities confirm the low densities of the Kepler-9 planets
- Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076
- A framework for the architecture of exoplanetary systems. I. Four classes of planetary system architecture
- The GTC exoplanet transit spectroscopy survey II: An overly-large Rayleigh-like feature for exoplanet TrES-3b
- The correlation between photometric variability and radial velocity jitter, based on TESS and HARPS observations
- Unbiasing the density of TTV-characterised sub-Neptunes: Update of the mass-radius relationship of 34 Kepler planets
- SimAb: A simple, fast and flexible model to assess the effects of planet formation on the atmospheric composition of gas giants
- A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS) -- IV. Candidate exoplanets around stars in open clusters: frequency and age-planetary radius distribution
- Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS
- Measuring precise radial velocities and cross-correlation function line-profile variations using a Skew Normal density
- MCMCI: A code to fully characterise an exoplanetary system
- The SOPHIE search for northern extrasolar planets-XIX. A system including a cold sub-Neptune potentially transiting a V = 6.5 star HD88986
- Characterisation of the Warm-Jupiter TOI-1130 system with CHEOPS and photo-dynamical approach
- Characterization of seven transiting systems including four warm Jupiters from SOPHIE and TESS
- TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS
- Photo-dynamical characterisation of the TOI-178 resonant chain
- Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396
- The GAPS Programme at TNG. LXV. Precise density measurement of TOI-1430 b, a young planet with an evaporating atmosphere
- Transit Timing Variations in HIP 41378: CHEOPS and TESS confirm a non-transiting sixth planet in the system