Dergi makalesi Açık Erişim
Basturk, Ozgur; Yalcinkaya, S.; Esmer, E. M.; Tanriverdi, T.; Mancini, L.; Daylan, T.; Southworth, J.; Keten, B.
{ "@context": "https://schema.org/", "@id": 4353, "@type": "ScholarlyArticle", "creator": [ { "@type": "Person", "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", "name": "Basturk, Ozgur" }, { "@type": "Person", "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", "name": "Yalcinkaya, S." }, { "@type": "Person", "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", "name": "Esmer, E. M." }, { "@type": "Person", "affiliation": "Nigde Omer Halisdemir Univ, Fac Arts & Sci, Dept Phys, TR-51240 Nigde, Turkey", "name": "Tanriverdi, T." }, { "@type": "Person", "name": "Mancini, L." }, { "@type": "Person", "name": "Daylan, T." }, { "@type": "Person", "affiliation": "Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England", "name": "Southworth, J." }, { "@type": "Person", "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", "name": "Keten, B." } ], "datePublished": "2020-01-01", "description": "We update the main physical and orbital properties of the transiting hot Saturn planet HAT-P-19 b, based on a global modelling of high-precision transit and occultation light curves, taken with ground-based and space telescopes, archive spectra and radial velocity measurements, brightness values from broad-band photometry, and Gaia parallax. We collected 65 light curves by amateur and professional observers, measured mid-transit times, and analysed their differences from calculated transit timings based on reference ephemeris information, which we update as a result. We have not found any periodicity in the residuals of a linear trend, which we attribute to the accumulation of uncertainties in the reference mid-transit time and the orbital period. We comment on the scenarios describing the formation and migration of this hot-Saturn type exoplanet with a bloated atmosphere yet a small core, although it is orbiting a metal-rich ([Fe/H] = 0.24 dex) host star. Finally, we review the planetary mass-radius, the orbital period-radius, and density, and the stellar metallicity-core mass diagrams, based on the parameters we derive for HAT-P-19 b and those of the other 70 transiting Saturn-mass planets from the NASA Exoplanet Archive.", "headline": "A holistic and probabilistic approach to the ground-based and spaceborne data of HAT-P-19 system", "identifier": 4353, "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", "license": "http://www.opendefinition.org/licenses/cc-by", "name": "A holistic and probabilistic approach to the ground-based and spaceborne data of HAT-P-19 system", "url": "https://aperta.ulakbim.gov.tr/record/4353" }
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