Kepler Eclipsing Binary Stars. I. Catalog and Principal Characterization of 1879 Eclipsing Binaries in the First Data Release
arXiv:1006.2815 · doi:10.1088/0004-6256/141/3/83
Abstract
The Kepler space mission is devoted to finding Earth-size planets in habitable zones orbiting other stars. Its large, 105-deg field-of-view features over 156,000 stars that are observed continuously to detect and characterize planet transits. Yet this high-precision instrument holds great promise for other types of objects as well. Here we present a comprehensive catalog of eclipsing binary stars observed by Kepler in the first 44 days of operation, the data which are publicly available through MAST as of 6/15/2010. The catalog contains 1879 unique objects. For each object we provide its Kepler ID (KID), ephemeris (BJD0, P0), morphology type, physical parameters (Teff, log g, E(B-V), crowding), and principal parameters (T2/T1, q, fillout factor and sin i for overcontacts, and T2/T1, (R1+R2)/a, e sin(w), e cos(w), and sin i for detached binaries). We present statistics based on the determined periods and measure an average occurence rate of eclipsing binaries to be ~1.2% across the Kepler field. We further discuss the distribution of binaries as function of galactic latitude, and thoroughly explain the application of artificial intelligence to obtain principal parameters in a matter of seconds for the whole sample. The catalog was envisioned to serve as a bridge between the now public Kepler data and the scientific community interested in eclipsing binary stars.
51 pages, in press (AJ). Online catalog: http://astro4.ast.villanova.edu/aprsa/kepler
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- Stellar statistics along the ecliptic and the impact on the K2 mission concept
- The SDSS-HET Survey of Kepler Eclipsing Binaries. A Sample of Four Benchmark Binaries
- The Detectability of Binary Star Planetary and Brown Dwarf Companions From Eclipse Timing Variations
- A Statistical Primer on Classical Period-Finding Techniques in Astronomy
- KIC 10417986: Spectroscopic confirmation of the nature of the binary system with a δ Scuti component
- First investigation of eclipsing binary KIC 9026766: analysis of light curve and periodic changes
- PSF-based Analysis for Detecting Unresolved Wide Binaries
- Confirmation of Seven Faint ATLAS Variable Star Candidates
- Circumbinary Planets -- The Next Steps
- Characteristics of Kepler Eclipsing Binaries Displaying a Significant O'Connell Effect
- Crowdfunding Astronomy Research with Google Sky
- Optimized cutting off transit algorithm to study stellar rotation from PLATO mission light curves
- A Minute-Cadence Deep Bulge Survey: First Data Release of DREAMS
- Kepler Pixel Project -- background RR Lyrae stars in the primary Kepler mission field of view
- Fractal Measures and Nonlinear Dynamics of Overcontact Binaries
- Recovering Signals in CoRoT Mission (RSCoRoT): I. Short Period Variable Stars
- The EBLM Project XVIII. 3D Obliquities of Five Low-Mass Eclipsing Binaries
- Detecting false positives with PLATO using double-aperture photometry and centroid shifts
- Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline
- Twinkle Twinkle Little Star, Roman Sees Where You Are: Predicting Exoplanet Transit Yields in the Rosette Nebula with the Nancy Grace Roman Space Telescope