High-precision photometry by telescope defocusing - III. The transiting planetary system WASP-2★: High-precision defocused photometry of WASP-2

[1]  A. Claret,et al.  A new non-linear limb-darkening law for LTE stellar atmosphere models III - Sloan filters: Calculations for –5.0 ≤ log [M/H] ≤ +1, 2000 K ≤ T$\mathsf{_{eff}}$ ≤ 50 000 K at several surface gravities , 2004 .

[2]  P. Maxted,et al.  Eclipsing binaries in open clusters – III. V621 Per in χ Persei , 2004, astro-ph/0409281.

[3]  R. G. West,et al.  Efficient identification of exoplanetary transit candidates from SuperWASP light curves , 2007, 0707.0417.

[4]  J. Jenkins,et al.  Some Tests to Establish Confidence in Planets Discovered by Transit Photometry , 2002 .

[5]  S. Seager,et al.  A Unique Solution of Planet and Star Parameters from an Extrasolar Planet Transit Light Curve , 2002, astro-ph/0206228.

[6]  Don A. VandenBerg,et al.  The Victoria-Regina Stellar Models: Evolutionary Tracks and Isochrones for a Wide Range in Mass and Metallicity that Allow for Empirically Constrained Amounts of Convective Core Overshooting , 2006 .

[7]  Th. Henning,et al.  Binarity of transit host stars - Implications for planetary parameters , 2009, 0902.2179.

[8]  P. Maxted,et al.  Eclipsing binaries in open clusters – I. V615 Per and V618 Per in h Persei , 2003, astro-ph/0312242.

[9]  A. Claret.  New grids of stellar models including tidal-evolution constants up to carbon burning - IV. From 0.8 to 125$M_{\odot}$: high metallicities (Z = 0.04–0.10) , 2007 .

[10]  Paul B. Etzel,et al.  A Simple Synthesis Method for Solving the Elements of Well-Detached Eclipsing Systems , 1981 .

[11]  Isaac Newton Group of Telescopes,et al.  Searching for transit timing variations in transiting exoplanet systems , 2008, Proceedings of the International Astronomical Union.

[12]  Burt Nelson,et al.  Eclipsing-Binary Solutions by Sequential Optimization of the Parameters , 1972 .

[13]  John Southworth,et al.  Homogeneous studies of transiting extrasolar planets – I. Light-curve analyses , 2008, 0802.3764.

[14]  R. Kurucz.  Model atmospheres for G, F, A, B, and O stars , 1979 .

[15]  David Charbonneau,et al.  The 3.6-8.0 μm Broadband Emission Spectrum of HD 209458b: Evidence for an Atmospheric Temperature Inversion , 2007, 0709.3984.

[16]  A. Claret,et al.  Absolute dimensions of detached eclipsing binaries – I. The metallic‐lined system WW Aurigae , 2005, astro-ph/0507629.

[17]  John Southworth,et al.  High-precision photometry by telescope defocussing - II. The transiting planetary system WASP-4 , 2009, 0907.3356.

[18]  Darko Jevremovic,et al.  The Dartmouth Stellar Evolution Database , 2008, 0804.4473.

[19]  A. Claret.  New grids of stellar models including tidal-evolution constants up to carbon burning. III. From 0.8 to 125 M: the Large Magellanic Cloud (Z = 0.007-0.01) , 2005 .

[20]  Mark S. Marley,et al.  Planetary Radii across Five Orders of Magnitude in Mass and Stellar Insolation: Application to Transits , 2006 .

[21]  A. Claret,et al.  New grids of stellar models including tidal-evolution constants up to carbon burning. III. From 0.8 , 2004 .

[22]  I. Baraffe,et al.  Structure and evolution of super-Earth to super-Jupiter exoplanets - I. Heavy element enrichment in the interior , 2008, 0802.1810.

[23]  A. Collier Cameron,et al.  H-band thermal emission from the 19-h period planet WASP-19b , 2010, 1002.1947.

[24]  J. Southworth.  Homogeneous studies of transiting extrasolar planets - II. Physical properties , 2008, 0811.3277.

[25]  P. Stetson.  DAOPHOT: A COMPUTER PROGRAM FOR CROWDED-FIELD STELLAR PHOTOMETRY , 1987 .

[26]  D. Buzasi,et al.  Eclipsing binaries observed with the WIRE satellite. I. Discovery and photometric analysis of the ne , 2006, astro-ph/0606551.

[27]  M. Holman,et al.  Accepted for publication in The Astrophysical Journal Preprint typeset using L ATEX style emulateapj v. 10/09/06 IMPROVED PARAMETERS FOR EXTRASOLAR TRANSITING PLANETS , 2008 .

[28]  P. J. Wheatley,et al.  High-precision photometry by telescope defocussing. I. The transiting planetary system WASP-5 , 2009, 0903.2139.

[29]  John Southworth,et al.  A method for the direct determination of the surface gravities of transiting extrasolar planets , 2007, 0704.1570.

[30]  G. Laughlin,et al.  On the Radii of Extrasolar Giant Planets , 2003 .

[31]  David Charbonneau,et al.  PRECISE RADIUS ESTIMATES FOR THE EXOPLANETS WASP-1b AND WASP-2b , 2007 .

[32]  Antonio Claret,et al.  The limb-darkening for spherically symmetric NextGen model atmospheres: A-G main-sequence and sub-giant stars , 2003 .

[33]  P. Maxted,et al.  Eclipsing binaries in open clusters. II. V453 Cyg in NGC 6871 , 2004, astro-ph/0403572.

[34]  W. Van Hamme,et al.  New limb-darkening coefficients for modeling binary star light curves , 1993 .

[35]  John Southworth,et al.  Eclipsing binaries observed with the WIRE satellite. II. beta Aurigae and non-linear limb darkening , 2007 .

[36]  L. Hebb,et al.  WASP-1b and WASP-2b: Two new transiting exoplanets detected with SuperWASP and SOPHIE , 2006, astro-ph/0609688.

[37]  P. Etzel,et al.  Photometric orbits of seven detached eclipsing binaries , 1981 .

[38]  A. Claret.  New grids of stellar models including tidal-evolution constants up to carbon burning. II. From 0.8 to 125 M: the Small Magellanic Cloud (Z = 0.002-0.004) , 2005 .

[39]  Richard S. Freedman,et al.  A Unified Theory for the Atmospheres of the Hot and Very Hot Jupiters: Two Classes of Irradiated Atmospheres , 2007, 0710.2558.

[40]  Jong-Hak Woo,et al.  Y2 Isochrones with an Improved Core Overshoot Treatment , 2004 .

[41]  S. Cassisi,et al.  A Large Stellar Evolution Database for Population Synthesis Studies. I. Scaled Solar Models and Isochrones , 2004, astro-ph/0405193.

[42]  G. Scarpetta,et al.  PHYSICAL PROPERTIES OF THE 0.94-DAY PERIOD TRANSITING PLANETARY SYSTEM WASP-18 , 2009, 0910.4875.