1 Ocak 2020 Dergi makalesi Açık Erişim

Basturk, Ozgur; Yalcinkaya, S.; Esmer, E. M.; Tanriverdi, T.; Mancini, L.; Daylan, T.; Southworth, J.; Keten, B.

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        "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", 
        "name": "Basturk, Ozgur"
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        "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", 
        "name": "Yalcinkaya, S."
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      {
        "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", 
        "name": "Esmer, E. M."
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      {
        "affiliation": "Nigde Omer Halisdemir Univ, Fac Arts & Sci, Dept Phys, TR-51240 Nigde, Turkey", 
        "name": "Tanriverdi, T."
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      {
        "name": "Mancini, L."
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      {
        "name": "Daylan, T."
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      {
        "affiliation": "Keele Univ, Astrophys Grp, Keele ST5 5BG, Staffs, England", 
        "name": "Southworth, J."
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        "affiliation": "Ankara Univ, Fac Sci, Astron & Space Sci Dept, TR-06100 Ankara, Turkey", 
        "name": "Keten, B."
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    "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.", 
    "doi": "10.1093/mnras/staa1758", 
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    "journal": {
      "issue": "4", 
      "pages": "4174-4190", 
      "title": "MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY", 
      "volume": "496"
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    "publication_date": "2020-01-01", 
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    "title": "A holistic and probabilistic approach to the ground-based and spaceborne data of HAT-P-19 system"
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