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Refining Parameters of the XO-5 Planetary System with High-Precision Transit Photometry

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Języki publikacji
EN
Abstrakty
EN
Studies of transiting extrasolar planets provide unique opportunity to get to know the internal structure of those worlds. The transiting exoplanet XO-5 b was found to have an anomalously high Safronov number and surface gravity. Our aim was to refine parameters of this intriguing system and search for signs of transit timing variations. We gathered high-precision light curves for two transits of XO-5 b. Assuming three different limb darkening laws, we found the best-fitting model and redetermined parameters of the system, including planet-to-star radius ratio, impact parameter and central time of transits. Error estimates were derived by the prayer bead method and Monte Carlo simulations. Although system's parameters obtained by us were found to agree with previous studies within one sigma, the planet was found to be notable smaller with the radius of 1.03+0.06-0.05 Jupiter radii. Our results confirm the high Safronov number and surface gravity of the planet. With two new mid-transit times, the ephemeris was refined to BJDTDB=(2454485.66842±0.00028)+(4.1877537±0.000017)E. No significant transit timing variation was detected.
Czasopismo
Rocznik
Strony
25--35
Opis fizyczny
Bibliogr. 33 poz., rys., tab., wykr.
Twórcy
  • Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, D-07745 Jena, Germany
  • Toruń Centre for Astronomy, N. Copernicus University, Gagarina 11, PL-87-100 Toruń, Poland
autor
  • Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, D-07745 Jena, Germany
autor
  • Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, D-07745 Jena, Germany
autor
  • Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, D-07745 Jena, Germany
  • Astrophysikalisches Institut und Universitäts-Sternwarte, Schillergässchen 2-3, D-07745 Jena, Germany
Bibliografia
  • Agol, E., Steffen, J., Sari, R., and Clarkson, W. 2005, MNRAS, 359, 567.
  • Burke, Ch., et al. 2008, ApJ, 686, 1331.
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  • Etzel, P.B. 1981, in: “Photometric and Spectroscopic Binary Systems”, Eds. Carling E.B., Kopal Z., NATO ASI Ser. C., 69, Kluwert, Dordrecht, 111.
  • Hansen, B.M.S., and Barman, T. 2007, ApJ, 671, 861.
  • Henry, G.W., Marcy, G.W., Butler, R.P., and Vogt, S.S. 2000, ApJ, 529, L41.
  • Holman, M.J., et al. 2010, Science, 330, 51.
  • Kipping, D.M. 2009, MNRAS, 392, 181.
  • Konacki, M., Torres, G., Jha, S., and Sasselov, D.D. 2003, Nature, 421, 507.
  • Maciejewski, G., et al. 2010, MNRAS, 407, 2625.
  • Maciejewski, G., et al. 2011, MNRAS, 411, 1204.
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  • Southworth, J. 2010, MNRAS, 408, 1689.
  • Southworth, J., Maxted, P.F.L., and Smalley, B. 2004a, MNRAS, 349, 547.
  • Southworth, J., Maxted, P.F.L., and Smalley, B. 2004b, MNRAS, 351, 1277.
  • Southworth, J., Wheatley, P.J., and Sams, G. 2007, MNRAS, 379, L11.
  • Southworth, J., et al. 2009, MNRAS, 396, 1023.
  • Southworth, J., et al. 2010, MNRAS, 408, 1680.
  • Van Hamme, W. 1993, AJ, 106, 2096.
  • Udalski, A., Kubiak, M., and Szymański, M. 1997, Acta Astron., 47, 319.
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  • Winn, J.N., et al. 2009, ApJ, 693, 794.
  • Zacharias, N., et al. 2004, A&AS, 205, 4815.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-adac763b-1414-473a-840b-facd7a1426e4
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