Qatar-1b: A hot Jupiter orbiting a metal-rich K dwarf star

K. A. Alsubai, N. R. Parley, D. M. Bramich, R. G. West, P. M. Sorensen, A. Collier Cameron, D. W. Latham, K. Horne, D. R. Anderson, G. Á Bakos, D. J.A. Brown, L. A. Buchhave, G. A. Esquerdo, M. E. Everett, G. Furész, J. D. Hartman, C. Hellier, G. M. Miller, D. Pollacco, S. N. QuinnJ. C. Smith, R. P. Stefanik, A. Szentgyorgyi

Research output: Contribution to journalArticle

40 Scopus citations

Abstract

We report the discovery and initial characterization of Qatar-1b, a hot Jupiter-orbiting metal-rich K dwarf star, the first planet discovered by the Qatar Exoplanet Survey. We describe the strategy used to select candidate transiting planets from photometry generated by the Qatar Exoplanet Survey camera array. We examine the rate of astrophysical and other false positives found during the spectroscopic reconnaissance of the initial batch of candidates. A simultaneous fit to the follow-up radial velocities and photometry of Qatar-1b yields a planetary mass of 1.09 ± 0.08MJ and a radius of 1.16 ± 0.05RJ. The orbital period and separation are 1.420033 ± 0.000016d and 0.02343 ± 0.00026au for an orbit assumed to be circular. The stellar density, effective temperature and rotation rate indicate an age greater than 4Gyr for the system.

Original languageEnglish (US)
Pages (from-to)709-716
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume417
Issue number1
DOIs
StatePublished - Oct 2011

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Planetary systems
  • Stars: individual: Qatar-1
  • Techniques: photometric
  • Techniques: radial velocities
  • Techniques: spectroscopic

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