MCMCI: A code to fully characterise an exoplanetary system
arXiv:1912.12632 · doi:10.1051/0004-6361/201936326
Abstract
Useful information can be retrieved by analysing the transit light curve of a planet-hosting star or induced radial velocity oscillations. However, inferring the physical parameters of the planet, such as mass, size, and semi-major axis, requires preliminary knowledge of some parameters of the host star, especially its mass or radius, which are generally inferred through theoretical evolutionary models. We seek to present and test a whole algorithm devoted to the complete characterisation of an exoplanetary system thanks to the global analysis of photometric or radial velocity time series combined with observational stellar parameters derived either from spectroscopy or photometry. We developed an integrated tool called MCMCI. This tool combines the Markov chain Monte Carlo (MCMC) approach of analysing photometric or radial velocity time series with a proper interpolation within stellar evolutionary isochrones and tracks, known as isochrone placement, to be performed at each chain step, to retrieve stellar theoretical parameters such as age, mass, and radius. We tested the MCMCI on the HD 219134 multi-planetary system hosting two transiting rocky super Earths and on WASP-4, which hosts a bloated hot Jupiter. Even considering different input approaches, a final convergence was reached within the code, we found good agreement with the results already stated in the literature and we obtained more precise output parameters, especially concerning planetary masses. The MCMCI tool offers the opportunity to perform an integrated analysis of an exoplanetary system without splitting it into the preliminary stellar characterisation through theoretical models. Rather this approach favours a close interaction between light curve analysis and isochrones, so that the parameters recovered at each step of the MCMC enter as inputs for purposes of isochrone placement.
18 pages, 6 figures, 6 tables. Accepted for publication in A&A. Source code link: https://github.com/Bonfanti88/MCMCI
References in corpus (89)
- emcee: The MCMC Hammer
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Gaia Data Release 2. Summary of the contents and survey properties
- PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
- Validation of the new Hipparcos reduction
- The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
- Analytic Lightcurves for Planetary Transit Searches
- MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones
- The K2 Mission: Characterization and Early results
- Accurate masses and radii of normal stars: modern results and applications
- Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics
- The PLATO 2.0 Mission
- batman: BAsic Transit Model cAlculatioN in Python
- A new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase
- Fast and scalable Gaussian process modeling with applications to astronomical time series
- Achieving better than 1 minute accuracy in the Heliocentric and Barycentric Julian Dates
- On the Unique Solution of Planet and Star Parameters from an Extrasolar Planet Transit Light Curve
- Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere
- Towards Better Age Estimates for Stellar Populations: The Y^2 Isochrones for Solar Mixture
- The CoRoT satellite in flight : description and performance
- EXOFAST: A fast exoplanetary fitting suite in IDL
- Improving PARSEC models for very low mass stars
- Origins of Hot Jupiters
- Stellar Diameters and Temperatures II. Main Sequence K & M Stars
- The Ages of Stars
- The effect of red noise on planetary transit detection
- Chromospheric CaII Emission in Nearby F, G, K, and M stars
- Improving the Efficiency of Markov Chain Monte Carlo for Analyzing the Orbits of Extrasolar Planets
- Quantifying the Uncertainty in the Orbits of Extrasolar Planets
- The 3.6-8.0 Micron Broadband Emission Spectrum of HD 209458b: Evidence for an Atmospheric Temperature Inversion
- Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler Mission
- Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog
- Juliet: a versatile modelling tool for transiting and non-transiting exoplanetary systems
- Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES-2
- Evolution of Thermally Pulsing Asymptotic Giant Branch Stars I. The COLIBRI Code
- The Broadband Infrared Emission Spectrum of the Exoplanet HD 189733b
- KELT-1b: A Strongly Irradiated, Highly Inflated, Short Period, 27 Jupiter-mass Companion Transiting a mid-F Star
- Kepler Flares II: The Temporal Morphology of White-Light Flares on GJ 1243
- A spin-down clock for cool stars from observations of a 2.5-billion-year-old cluster
- CHEOPS: A Transit Photometry Mission for ESA's Small Mission Programme
- Oxygen Abundances in Nearby FGK Stars and the Galactic Chemical Evolution of the Local Disk and Halo
- CLES, Code Liegeois d'Evolution Stellaire
- Periodic Flux Variability of Stars due to the Reflex Doppler Effect Induced by Planetary Companions
- The Transit Light Curve (TLC) Project. I. Four Consecutive Transits of the Exoplanet XO-1b
- The TRAPPIST survey of southern transiting planets. I. Thirty eclipses of the ultra-short period planet WASP-43 b
- Isochrone ages for field dwarfs: method and application to the age-metallicity relation
- Starspots and spin-orbit alignment in the WASP-4 exoplanetary system
- Vertical distribution of Galactic disk stars IV - AMR and AVR from clump giants
- The atmospheric parameters and spectral interpolator for the stars of MILES
- Line-profile tomography of exoplanet transits I: The Doppler shadow of HD 189733b
- Asteroseismology for "à la carte" stellar age-dating and weighing: Age and mass of the CoRoT exoplanet host HD 52265
- The influence of atomic diffusion on stellar ages and chemical tagging
- Improved parameters for the transiting hot Jupiters WASP-4b and WASP-5b
- The HARPS-N Rocky Planet Search I. HD219134b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun
- WASP-4b: a 12th-magnitude transiting hot-Jupiter in the Southern hemisphere
- The Photoeccentric Effect and Proto-Hot Jupiters I. Measuring photometric eccentricities of individual transiting planets
- WASP-30b: a 61 Mjup brown dwarf transiting a V=12, F8 star
- The thermal emission of the young and massive planet CoRoT-2b at 4.5 and 8 microns
- The TESS-HERMES survey Data Release 1: high-resolution spectroscopy of the TESS southern continuous viewing zone
- Age consistency between exoplanet hosts and field stars
- Towards precise stellar ages: combining isochrone fitting with empirical gyrochronology
- Revising the ages of planet-hosting stars
- Accurate and homogeneous abundance patterns in solar-type stars of the solar neighbourhood: a chemo-chronological analysis
- Heavy Element Diffusion in Metal Poor Stars
- Pyaneti: a fast and powerful software suite for multi-planet radial velocity and transit fitting
- The Transit Light Curve Project. XI. Submillimagnitude Photometry of Two Transits of the Bloated Planet WASP-4b
- VLT transit and occultation photometry for the bloated planet CoRoT-1b
- Two massive rocky planets transiting a K-dwarf 6.5 parsecs away
- High-precision abundances of Sc, Mn, Cu, and Ba in solar twins. Trends of element ratios with stellar age
- High-precision photometry by telescope defocussing. II. The transiting planetary system WASP-4
- WASP-4b Arrived Early for the TESS Mission
- On the metallicity dependance of the [Y/Mg] - age relation for solar type stars
- Empirical Constraints on Trojan Companions and Orbital Eccentricities in 25 Transiting Exoplanetary Systems
- Secondary Eclipse Photometry of WASP-4b with Warm Spitzer
- Evolution of Thermally Pulsing Asymptotic Giant Branch Stars V: Constraining the Mass Loss and Lifetimes of Intermediate Mass, Low Metallicity AGB Stars
- Determining Eccentricities of Transiting Planets: A Divide in the Mass-Period Plane
- A Six-Planet System Orbiting HD 219134
- Interferometric diameters of five evolved intermediate-mass planet-hosting stars measured with PAVO at the CHARA Array
- A Model of Magnetic Braking of Solar Rotation That Satisfies Observational Constraints
- HATS-60b - HATS-69b: Ten Transiting Planets From HATSouth
- WASP-50b: a hot Jupiter transiting a moderately active solar-type star
- K2-99: a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion
- The [Y/Mg] clock works for evolved solar metallicity stars
- Tidal decay and orbital circularization in close-in two-planet systems
- Constraints on the structure of 16 Cyg A and 16 Cyg B using inversion techniques
- WASP-4b Transit Observations With GROND
- Radial Velocities as an Exoplanet Discovery Method
- PlanetPack3: a radial-velocity and transit analysis tool for exoplanets
- Tidal decay and circularization of the orbits of short-period planets
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- pyaneti II: A multidimensional Gaussian process approach to analysing spectroscopic time-series
- 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
- Detection of the tidal deformation of WASP-103b at with CHEOPS
- A framework for the architecture of exoplanetary systems. I. Four classes of planetary system architecture
- Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N and TESS
- SPInS, a pipeline for massive stellar parameter inference: A public Python tool to age-date, weigh, size up stars, and more
- TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS
- Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396
- More planetary candidates from K2 Campaign 5 by tran_k2
- NLTE atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations
- From Global Climate Models (GCMs) to Exoplanet Spectra with the Global Emission Spectra (GlobES)
- The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
- Discovery of a young low-mass brown dwarf transiting a fast-rotating F-type star by the Galactic Plane eXoplanet (GPX) survey