High-precision photometry by telescope defocusing - III. The transiting planetary system WASP-2

November 2010 • 2010MNRAS.408.1680S

Authors • Southworth, John • Mancini, L. • Novati, S. Calchi • Dominik, M. • Glitrup, M. • Hinse, T. C. • Jørgensen, U. G. • Mathiasen, M. • Ricci, D. • Maier, G. • Zimmer, F. • Bozza, V. • Browne, P. • Bruni, I. • Burgdorf, M. • Dall'Ora, M. • Finet, F. • Harpsøe, K. • Hundertmark, M. • Liebig, C. • Rahvar, S. • Scarpetta, G. • Skottfelt, J. • Smalley, B. • Snodgrass, C. • Surdej, J.

Abstract • We present high-precision photometry of three transits of the extrasolar planetary system WASP-2, obtained by defocusing the telescopes, and achieving scatters of between 0.42 and 0.73 mmag versus the best-fitting model. These data are modelled using the JKTEBOP code, and taking into account the light from the recently discovered faint star close to the system. The physical properties of the WASP-2 system are derived using tabulated predictions from five different sets of stellar evolutionary models, allowing both statistical and systematic error bars to be specified. We find the mass and radius of the planet to be M_b = 0.846 +/- 0.055 +/- 0.023M_Jup and R_b = 1.043 +/- 0.029 +/- 0.015R_Jup. It has a low equilibrium temperature of 1281 +/- 21K, in agreement with a recent finding that it does not have an atmospheric temperature inversion. The first of our transit data sets has a scatter of only 0.42mmag with respect to the best-fitting light-curve model, which to our knowledge is a record for ground-based observations of a transiting extrasolar planetary system.

Based on data collected by MiNDSTEp with the Danish 1.54-m telescope at the ESO La Silla Observatory.

E-mail: jkt@astro.keele.ac.uk ‡

Royal Society University Research Fellow.

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Sebastiano Calchi Novati

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