TASTE IV: Refining ephemeris and orbital parameters for HAT‐P‐20b and WASP‐1b. Issue 8 (October 2014)

• Record Type: Journal Article
• Authors: Granata, V.; Nascimbeni, V.; Piotto, G.; Bedin, L. R.; Borsato, L.; Cunial, A.; Damasso, M.; Malavolta, L.
• Is Part Of: Astronomische Nachrichten. Volume 335:Issue 8(2014)
• Page Start: 797
• Page End: 803
• Publication Date: 2014-10
• Subjects: Astronomy -- Periodicals; 520.5
• DOI: 10.1002/asna.201412072
• Languages: English
• ISSNs: 0004-6337

Abstract

<abstract abstract-type="main" xml:lang="en"> <title>Abstract</title> <p>We present four new light curves of the transiting exoplanets WASP‐1b and HAT‐P‐20b, observed within the TASTE (The Asiago Search for Transit timing variations of Exoplanets) project. We re‐analyzed light curves from the literature in a homogeneous way, calculating a refined ephemeris and orbital‐physical parameters for both objects. WASP‐1b does not show any significant Transit Timing Variation signal at the 120 s level. As for HAT‐P‐20b, we detected a deviation from our re‐estimated linear ephemeris that could be ascribed to the presence of a perturber or, more probably, to a previously unnoticed high level of stellar activity. The rotational period of HAT‐P‐20 A that we obtained from archival data (<italic>P</italic>_rot ≃ 14.5 d), combined with its optical variability and strong emission of Ca ii H &amp; K lines, is consistent with a young stellar age (&lt;1 Gyr) and support the hypothesis that stellar activity may be responsible of the measured deviations of the transit times. (© 2014 WILEY‐VCH Verlag GmbH &amp; Co. KGaA, Weinheim)</p> </abstract>