MODELING KEPLER TRANSIT LIGHT CURVES AS FALSE POSITIVES: REJECTION OF BLEND SCENARIOS FOR KEPLER-9, AND VALIDATION OF KEPLER-9 d, A SUPER-EARTH-SIZE PLANET IN A MULTIPLE SYSTEM
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Howard Isaacson | David G. Monet | David Charbonneau | William F. Welsh | Jon M. Jenkins | Edward W. Dunham | Timothy M. Brown | Stephen T. Bryson | Jason H. Steffen | Eric B. Ford | William J. Borucki | David G. Koch | Natalie M. Batalha | Jack J. Lissauer | Steve B. Howell | Darin Ragozzine | Andrej Prsa | Jason F. Rowe | Guillermo Torres | Daniel C. Fabrycky | Dimitar D. Sasselov | David W. Latham | David R. Ciardi | Ronald L. Gilliland | Geoffrey W. Marcy | Matthew J. Holman | Lars A. Buchhave | F. Fressin | E. Ford | D. Monet | M. Holman | J. Lissauer | R. Gilliland | T. Brown | D. Ciardi | L. Buchhave | D. Latham | D. Sasselov | D. Charbonneau | G. Marcy | H. Isaacson | J. Rowe | J. Jenkins | S. Bryson | S. Howell | N. Batalha | S. Quinn | W. Borucki | D. Koch | G. Torres | J. Steffen | D. Fabrycky | W. Welsh | A. Prša | E. Dunham | D. Ragozzine | Thomas N. Gautier | Franccois Fressin | T. N. Gautier III
[1] G. L. Wycoff,et al. The Second US Naval Observatory CCD Astrograph Catalog (UCAC2) , 2004, astro-ph/0403060.
[2] Francois Fressin,et al. Interpreting and predicting the yield of transit surveys: Giant planets in the OGLE fields , 2007, 0704.1919.
[3] F. Bouchy,et al. The HARPS search for southern extra-solar planets: XVIII. An Earth-mass planet in the GJ 581 planetary system , 2009, 0906.2780.
[4] Howard Isaacson,et al. The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters , 2010, Science.
[5] Paul B. Etzel,et al. A Simple Synthesis Method for Solving the Elements of Well-Detached Eclipsing Systems , 1981 .
[6] Radius and Structure Models of the First Super-Earth Planet , 2006, astro-ph/0610122.
[7] et al,et al. The CoRoT space mission : early results Special feature Transiting exoplanets from the CoRoT space mission VIII . CoRoT-7 b : the first super-Earth with measured radius , 2009 .
[8] Howard Isaacson,et al. Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations , 2010, Science.
[9] P. Etzel,et al. Photometric orbits of seven detached eclipsing binaries , 1981 .
[10] I. King,et al. Accuracy of measurement of star images on a pixel array , 1983 .
[11] Willy Benz,et al. Extrasolar planet population synthesis I: Method, formation tracks and mass-distance distribution , 2009, 0904.2524.
[12] T. Guillot,et al. Interpreting the yield of transit surveys: are there groups in the known transiting planets population? , 2009 .
[13] M. R. Haas,et al. Kepler Mission Design, Realized Photometric Performance, and Early Science , 2010, 1001.0268.
[14] C. Moutou,et al. Improved stellar parameters of CoRoT-7 A star hosting two super Earths , 2010, 1005.3208.
[15] S. Baliunas,et al. No Planet for Hd 166435 , 2022 .
[16] F. Bouchy,et al. Towards the characterization of the hot Neptune/super-Earth population around nearby bright stars , 2008, Proceedings of the International Astronomical Union.
[17] D. Lin,et al. Toward a Deterministic Model of Planetary Formation. I. A Desert in the Mass and Semimajor Axis Distributions of Extrasolar Planets , 2004 .
[18] E. B. Carling,et al. Photometric and Spectroscopic Binary Systems , 1981 .
[19] A. Prsa,et al. PRE-SPECTROSCOPIC FALSE-POSITIVE ELIMINATION OF KEPLER PLANET CANDIDATES , 2010, 1001.0392.
[20] Xavier Bonfils,et al. A super-Earth transiting a nearby low-mass star , 2009, Nature.
[21] Belgium,et al. Evolution of asymptotic giant branch stars. II. Optical to far-infrared isochrones with improved TP- , 2007, 0711.4922.
[22] Burt Nelson,et al. Eclipsing-Binary Solutions by Sequential Optimization of the Parameters , 1972 .
[23] F. Fressin,et al. FIVE KEPLER TARGET STARS THAT SHOW MULTIPLE TRANSITING EXOPLANET CANDIDATES , 2010, 1006.2763.
[24] M. Couture,et al. HIRES: the high-resolution echelle spectrometer on the Keck 10-m Telescope , 1994, Astronomical Telescopes and Instrumentation.
[25] E. Agol,et al. Analytic Light Curves for Planetary Transit Searches , 2002, astro-ph/0210099.
[26] David K. Sing,et al. Stellar limb-darkening coefficients for CoRot and Kepler , 2009, 0912.2274.
[27] David G. Monet,et al. Preliminary Astrometric Results from Kepler , 2010, 1001.0305.
[28] Howard Isaacson,et al. Kepler Planet-Detection Mission: Introduction and First Results , 2010, Science.
[29] A. Sozzetti,et al. HD 147506b: A Supermassive Planet in an Eccentric Orbit Transiting a Bright Star , 2007, 0705.0126.
[30] David Charbonneau,et al. The Challenge of Wide-Field Transit Surveys: The Case of GSC 01944-02289 , 2005, astro-ph/0501554.
[31] David Charbonneau,et al. Rejecting Astrophysical False Positives from the TrES Transiting Planet Survey: The Example of GSC 03885–00829 , 2006 .
[32] J. Zahn,et al. Tidal Effects in Stars, Planets and Disks , 2008 .
[33] G. Kotliar,et al. Orbital selective and tunable Kondo effect of magnetic adatoms on graphene: Correlated electronic structure calculations , 2010, 1006.2779.
[34] Berkeley,et al. TESTING BLEND SCENARIOS FOR EXTRASOLAR TRANSITING PLANET CANDIDATES. I. OGLE-TR-33: A FALSE POSITIVE , 2004 .
[35] Berkeley,et al. Testing Blend Scenarios for Extrasolar Transiting Planet Candidates. II. OGLE-TR-56 , 2005 .
[36] Howard Isaacson,et al. DISCOVERY AND ROSSITER–McLAUGHLIN EFFECT OF EXOPLANET KEPLER-8b , 2010, 1001.0416.
[37] A. Robin,et al. A synthetic view on structure and evolution of the Milky Way , 2003 .
[38] J. Mathis,et al. The relationship between infrared, optical, and ultraviolet extinction , 1989 .