CHEOPS observations of the HD 108236 planetary system: a fifth planet, improved ephemerides, and planetary radii
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J. Laskar | V. Adibekyan | S. Barros | M. Deleuil | O. Demangeon | N. Santos | D. Ehrenreich | F. Wildi | S. Udry | R. Ragazzoni | J. Farinato | N. Walton | W. Benz | D. Futyan | A. Bonfanti | Wolfgang Baumjohann | H. Michaelis | A. Cameron | G. Piotto | C. Lovis | T. Wilson | Y. Alibert | T. Bandy | C. Broeg | E. Pall'e | D. S'egransan | S. Sousa | V. Nascimbeni | I. Pagano | G. Scandariato | D. Barrado | T. Kuntzer | B. Demory | X. Bonfils | V. Grootel | M. Gillon | L. Delrez | K. Heng | D. Queloz | D. Pollacco | J. Cabrera | D. Gandolfi | H. Rauer | A. Erikson | V. V. Eylen | I. Ribas | M. Fridlund | C. Persson | H. Osborn | M. Davies | S. Charnoz | M. Salatti | D. Wolter | I. Walter | N. Rando | D. Magrin | L. Kiss | S. Salmon | A. Fortier | M. Steller | N. Thomas | L. Fossati | L. Borsato | K. Isaak | A. Muñoz | G. Peter | B. Chazelas | G. Szab'o | L. Marafatto | R. Rohlfs | N. Billot | A. Brandeker | R. Ottensamer | S. Hoyer | O. Barrag'an | A. Bekkelien | M. Lendl | P. Guterman | M. Guedel | P. Maxted | A.M.S. Smith | M. Hooton | A. Tuson | M. Bergomi | D. Piazza | V. Viotto | G. Olofsson | A. Mustill | G. Lacedelli | M. Munari | R. Alonso | J. Asquier | T. B'arczy | M. Beck | T. Beck | M. Busch | V. Cessa | C. V. Damme | J. Hasiba | E. Hernandez | L. Malvasio | H. Ottacher | F. Ratti | M. Rieder | F. Safa | A. Simon | M. Sordet | M. Tschentscher | A. D. Étangs | A. Smith | A. G. Muñoz
[1] J. L. Rasilla,et al. ESPRESSO at VLT , 2020 .
[2] H. Lammer,et al. Hydrogen Dominated Atmospheres on Terrestrial Mass Planets: Evidence, Origin and Evolution , 2020, Space Science Reviews.
[3] J. Laskar,et al. The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS , 2020, Astronomy & Astrophysics.
[4] E. Ford,et al. Architectures of Exoplanetary Systems. III. Eccentricity and Mutual Inclination Distributions of AMD-stable Planetary Systems , 2020, The Astronomical Journal.
[5] Constantinos Marios Angelopoulos,et al. DHP Framework: Digital Health Passports Using Blockchain - Use case on international tourism during the COVID-19 pandemic , 2020, ArXiv.
[6] P. C. Thao,et al. TESS Hunt for Young and Maturing Exoplanets (THYME). III. A Two-planet System in the 400 Myr Ursa Major Group , 2020, The Astronomical Journal.
[7] Chelsea X. Huang,et al. TESS Discovery of a Super-Earth and Three Sub-Neptunes Hosted by the Bright, Sun-like Star HD 108236 , 2020, The Astronomical Journal.
[8] R. P. Butler,et al. The Multiplanet System TOI-421: A Warm Neptune and a Super Puffy Mini-Neptune Transiting a G9 V Star in a Visual Binary , 2020, The Astronomical Journal.
[9] J. Owen,et al. Testing exoplanet evaporation with multitransiting systems , 2019, Monthly Notices of the Royal Astronomical Society.
[10] M. Davies,et al. The Kepler-11 system: evolution of the stellar high-energy emission and initial planetary atmospheric mass fractions , 2019, Astronomy & Astrophysics.
[11] D. Kipping,et al. The multiplicity distribution of Kepler’s exoplanets , 2019, Monthly Notices of the Royal Astronomical Society.
[12] Chelsea X. Huang,et al. A Super-Earth and Sub-Neptune Transiting the Late-type M Dwarf LP 791-18 , 2019, The Astrophysical Journal.
[13] Sara Seager,et al. Securing the Legacy of TESS through the Care and Maintenance of TESS Planet Ephemerides , 2019, The Astronomical Journal.
[14] Adam L. Kraus,et al. TESS Spots a Compact System of Super-Earths around the Naked-eye Star HR 858 , 2019, The Astrophysical Journal.
[15] E. Lopez,et al. The Sub-Neptune Desert and Its Dependence on Stellar Type: Controlled by Lifetime X-Ray Irradiation , 2019, The Astrophysical Journal.
[16] J. Speagle. dynesty: a dynamic nested sampling package for estimating Bayesian posteriors and evidences , 2019, Monthly Notices of the Royal Astronomical Society.
[17] H. Lammer,et al. Close-in Sub-Neptunes Reveal the Past Rotation History of Their Host Stars: Atmospheric Evolution of Planets in the HD 3167 and K2-32 Planetary Systems , 2019, Astrophysical Journal.
[18] Keivan G. Stassun,et al. The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf , 2019, The Astronomical Journal.
[19] Keivan G. Stassun,et al. The Transiting Multi-planet System HD15337: Two Nearly Equal-mass Planets Straddling the Radius Gap , 2019, The Astrophysical Journal.
[20] Yann Alibert,et al. New metric to quantify the similarity between planetary systems: application to dimensionality reduction using T-SNE , 2019, Astronomy & Astrophysics.
[21] Keivan G. Stassun,et al. Near-resonance in a System of Sub-Neptunes from TESS , 2019, The Astronomical Journal.
[22] Keivan G. Stassun,et al. TESS Delivers Its First Earth-sized Planet and a Warm Sub-Neptune , 2018, The Astrophysical Journal.
[23] H. Lammer,et al. Grid of upper atmosphere models for 1–40 M⊕ planets: application to CoRoT-7 b and HD 219134 b,c , 2018, Astronomy & Astrophysics.
[24] D. Gandolfi,et al. pyaneti: a fast and powerful software suite for multiplanet radial velocity and transit fitting , 2018, Monthly Notices of the Royal Astronomical Society.
[25] Maxwell X. Cai,et al. The Orbital Eccentricity of Small Planet Systems , 2018, The Astronomical Journal.
[26] K. Stassun,et al. Evidence for a Systematic Offset of −80 μas in the Gaia DR2 Parallaxes , 2018, The Astrophysical Journal.
[27] T. A. Lister,et al. Gaia Data Release 2. Summary of the contents and survey properties , 2018, 1804.09365.
[28] P. Maxted. Comparison of the power-2 limb-darkening law from the STAGGER-grid to Kepler light curves of transiting exoplanets , 2018, Astronomy & Astrophysics.
[29] Clea F. Schumer,et al. 275 Candidates and 149 Validated Planets Orbiting Bright Stars in K2 Campaigns 0–10 , 2018, 1802.05277.
[30] F. Timmes,et al. Modules for Experiments in Stellar Astrophysics ( ): Convective Boundaries, Element Diffusion, and Massive Star Explosions , 2017, 1710.08424.
[31] Andrew Cumming,et al. The California-Kepler Survey. V. Peas in a Pod: Planets in a Kepler Multi-planet System Are Similar in Size and Regularly Spaced , 2017, 1706.06204.
[32] Christoph Mordasini,et al. Compositional Imprints in Density–Distance–Time: A Rocky Composition for Close-in Low-mass Exoplanets from the Location of the Valley of Evaporation , 2017, 1706.00251.
[33] James E. Owen,et al. The Evaporation Valley in the Kepler Planets , 2017, 1705.10810.
[34] Howard Isaacson,et al. The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets , 2017, 1703.10375.
[35] Daniel Foreman-Mackey,et al. Fast and Scalable Gaussian Process Modeling with Applications to Astronomical Time Series , 2017, 1703.09710.
[36] S. Raymond,et al. Breaking the chains: hot super-Earth systems from migration and disruption of compact resonant chains , 2017, 1703.03634.
[37] L. Girardi,et al. A NEW GENERATION OF PARSEC-COLIBRI STELLAR ISOCHRONES INCLUDING THE TP-AGB PHASE , 2017, 1701.08510.
[38] Nate B. Lust,et al. ON CORRELATED-NOISE ANALYSES APPLIED TO EXOPLANET LIGHT CURVES , 2016, 1610.01336.
[39] A. Johansen,et al. The effects of external planets on inner systems: multiplicities, inclinations and pathways to eccentric warm Jupiters , 2016, 1609.08058.
[40] Christoph Baranec,et al. FIVE PLANETS TRANSITING A NINTH MAGNITUDE STAR , 2016, 1606.08441.
[41] J. Valenti,et al. Spectroscopy Made Easy: Evolution , 2016, 1606.06073.
[42] Jieun Choi,et al. MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS , 2016, 1604.08592.
[43] D. Kipping,et al. PROBABILISTIC FORECASTING OF THE MASSES AND RADII OF OTHER WORLDS , 2016, 1603.08614.
[44] P. Maxted. ELLC - a fast, flexible light curve model for detached eclipsing binary stars and transiting exoplanets , 2016, 1603.08484.
[45] H. Rein,et al. Second-order variational equations for N-body simulations , 2016, 1603.03424.
[46] Aaron Dotter,et al. MESA ISOCHRONES AND STELLAR TRACKS (MIST) 0: METHODS FOR THE CONSTRUCTION OF STELLAR ISOCHRONES , 2016, 1601.05144.
[47] Khadeejah A. Zamudio,et al. PLANETARY CANDIDATES OBSERVED BY KEPLER. VII. THE FIRST FULLY UNIFORM CATALOG BASED ON THE ENTIRE 48-MONTH DATA SET (Q1–Q17 DR24) , 2015, 1512.06149.
[48] H. Lammer,et al. THE EVOLUTION OF STELLAR ROTATION AND THE HYDROGEN ATMOSPHERES OF HABITABLE-ZONE TERRESTRIAL PLANETS , 2015, 1511.03647.
[49] A. Bonfanti,et al. Age consistency between exoplanet hosts and field stars , 2015, 1511.01744.
[50] C. Unterborn,et al. SCALING THE EARTH: A SENSITIVITY ANALYSIS OF TERRESTRIAL EXOPLANETARY INTERIOR MODELS , 2015, 1510.07582.
[51] M. Tsantaki,et al. Identifying the best iron-peak and α-capture elements for chemical tagging: The impact of the number of lines on measured scatter , 2015, 1509.02419.
[52] A. Santerne,et al. Constraining planet structure from stellar chemistry : the cases of CoRoT-7, Kepler-10, and Kepler-93 , 2015, 1507.08081.
[53] Y. Alibert,et al. Elemental ratios in stars vs planets (Research Note) , 2015, 1507.01343.
[54] Hanno Rein,et al. WHFAST: a fast and unbiased implementation of a symplectic Wisdom-Holman integrator for long-term gravitational simulations , 2015, 1506.01084.
[55] S. Albrecht,et al. ECCENTRICITY FROM TRANSIT PHOTOMETRY: SMALL PLANETS IN KEPLER MULTI-PLANET SYSTEMS HAVE LOW ECCENTRICITIES , 2015, 1505.02814.
[56] S. G. Sousa,et al. ARES v2 - new features and improved performance , 2015, 1504.02725.
[57] E. Dorfi,et al. Hydrodynamic simulations of captured protoatmospheres around Earth-like planets , 2015, 1505.06859.
[58] M. Gudel,et al. Stellar winds on the main-sequence - II. The evolution of rotation and winds , 2015, 1503.07494.
[59] A. Jord'an,et al. Limb darkening and exoplanets: testing stellar model atmospheres and identifying biases in transit parameters , 2015, 1503.07020.
[60] Yanqin Wu,et al. Spacing of Kepler Planets: Sculpting by Dynamical Instability , 2015, 1502.05449.
[61] P. Tackley,et al. Can we constrain the interior structure of rocky exoplanets from mass and radius measurements , 2015, 1502.03605.
[62] C. Baranec,et al. AN ANCIENT EXTRASOLAR SYSTEM WITH FIVE SUB-EARTH-SIZE PLANETS , 2015, 1501.06227.
[63] A. Bonfanti,et al. Revising the ages of planet-hosting stars , 2014, 1411.4302.
[64] Joshua N. Winn,et al. The Occurrence and Architecture of Exoplanetary Systems , 2014, 1410.4199.
[65] S. Sousa. ARES + MOOG: A Practical Overview of an Equivalent Width (EW) Method to Derive Stellar Parameters , 2014, 1407.5817.
[66] Mark Clampin,et al. Transiting Exoplanet Survey Satellite , 2014, 1406.0151.
[67] D. Kipping. Efficient, uninformative sampling of limb darkening coefficients for two-parameter laws , 2013, 1308.0009.
[68] M. P. Hobson,et al. Importance Nested Sampling and the MultiNest Algorithm , 2013, The Open Journal of Astrophysics.
[69] D. Queloz,et al. CHEOPS: A transit photometry mission for ESA's small mission programme , 2013, 1305.2270.
[70] L. Girardi,et al. parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code , 2012, 1208.4498.
[71] J. Laskar,et al. Dissipation in planar resonant planetary systems , 2012, 1207.3171.
[72] V. Adibekyan,et al. Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program - Galactic stellar populations and planets , 2012, 1207.2388.
[73] John C. Geary,et al. ARCHITECTURE OF KEPLER'S MULTI-TRANSITING SYSTEMS. II. NEW INVESTIGATIONS WITH TWICE AS MANY CANDIDATES , 2012, The Astrophysical Journal.
[74] Daniel Foreman-Mackey,et al. emcee: The MCMC Hammer , 2012, 1202.3665.
[75] H. Rein,et al. REBOUND: An open-source multi-purpose N-body code for collisional dynamics , 2011, 1110.4876.
[76] Nicholas J. Wright,et al. THE STELLAR-ACTIVITY–ROTATION RELATIONSHIP AND THE EVOLUTION OF STELLAR DYNAMOS , 2011, 1109.4634.
[77] I. Ribas,et al. Estimation of the XUV radiation onto close planets and their evaporation , 2011, 1105.0550.
[78] S. Bloemen,et al. Gravity and limb-darkening coefficients for the Kepler, CoRoT, Spitzer, uvby, UBVRIJHK, and Sloan photometric systems , 2011 .
[79] Jon M. Jenkins,et al. ARCHITECTURE AND DYNAMICS OF KEPLER'S CANDIDATE MULTIPLE TRANSITING PLANET SYSTEMS , 2011, 1102.0543.
[80] J. Winn. Exoplanet Transits and Occultations , 2010 .
[81] Martin G. Cohen,et al. THE WIDE-FIELD INFRARED SURVEY EXPLORER (WISE): MISSION DESCRIPTION AND INITIAL ON-ORBIT PERFORMANCE , 2010, 1008.0031.
[82] Ryan M. Ferguson,et al. THE JINA REACLIB DATABASE: ITS RECENT UPDATES AND IMPACT ON TYPE-I X-RAY BURSTS , 2010, The Astrophysical Journal Supplement Series.
[83] A. B. Balantekin,et al. Solar fusion cross sections II: the pp chain and CNO cycles , 2010, 1004.2318.
[84] David P. O'Brien,et al. THE COMPOSITIONAL DIVERSITY OF EXTRASOLAR TERRESTRIAL PLANETS. I. IN SITU SIMULATIONS , 2010, 1004.0971.
[85] Bernd Freytag,et al. Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere , 2010, 1003.1190.
[86] Sean N. Raymond,et al. GENERALIZED MILANKOVITCH CYCLES AND LONG-TERM CLIMATIC HABITABILITY , 2010, 1002.4877.
[87] M. Asplund,et al. The chemical composition of the Sun , 2009, 0909.0948.
[88] A. Gimenez,et al. Accurate masses and radii of normal stars: modern results and applications , 2009, 0908.2624.
[89] Austria,et al. Low-temperature gas opacity. ÆSOPUS: a versatile and quick computational tool , 2009, 0907.3248.
[90] L. Hillenbrand,et al. Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics , 2008, 0807.1686.
[91] D. Queloz,et al. Spectroscopic parameters for 451 stars in the HARPS GTO planet search program - Stellar [Fe/H] and the frequency of exo-Neptunes , 2008, 0805.4826.
[92] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[93] R. Scuflaire,et al. CLÉS, Code Liégeois d’Évolution Stellaire , 2007, 0712.3471.
[94] F. Feroz,et al. Multimodal nested sampling: an efficient and robust alternative to Markov Chain Monte Carlo methods for astronomical data analyses , 2007, 0704.3704.
[95] Porto,et al. A new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES) , 2007, astro-ph/0703696.
[96] M. Skrutskie,et al. The Two Micron All Sky Survey (2MASS) , 2006 .
[97] Christopher K. I. Williams,et al. Gaussian Processes for Machine Learning (Adaptive Computation and Machine Learning) , 2005 .
[98] Matthew J. Holman,et al. The Use of Transit Timing to Detect Terrestrial-Mass Extrasolar Planets , 2005, Science.
[99] David R. Alexander,et al. Low-Temperature Opacities , 2005, astro-ph/0502045.
[100] Carles Simó,et al. Phase space structure of multi-dimensional systems by means of the mean exponential growth factor of nearby orbits , 2003 .
[101] E. Ford. Quantifying the Uncertainty in the Orbits of Extrasolar Planets , 2003, astro-ph/0305441.
[102] Forrest J. Rogers,et al. Updated Opal Opacities , 1996 .
[103] M. J. Shallis,et al. Stellar angular diameters from infrared photometry. Application to Arcturus and other stars; with effective temperatures. , 1977 .
[104] N. Pizzolato,et al. The stellar activity-rotation relationship revisited: Dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfs ? , 2003 .
[105] Jordi MIRALDA-ESCUDEç. ORBITAL PERTURBATIONS OF TRANSITING PLANETS: A POSSIBLE METHOD TO MEASURE STELLAR QUADRUPOLES AND TO DETECT EARTH-MASS PLANETS , 2002 .
[106] Robert L. Kurucz,et al. SYNTHE Spectrum Synthesis Programs and Line Data. , 1993 .