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The HoSTS Project: A Homogeneous Study of Transiting Systems

Published online by Cambridge University Press:  06 January 2014

Yilen Gómez Maqueo Chew ,
Francesca Faedi ,
Leslie Hebb ,
Don Pollacco ,
Keivan Stassun ,
Phillip Cargile ,
Barry Smalley ,
Amanda Doyle ,
Luan Ghezzi  and
Susana C. C. Barros
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Yilen Gómez Maqueo Chew
Affiliation:
Department of Physics & Astronomy, Vanderbilt University, Nashville, TN 37235, USA Department of Physics, University of Warwick, Coventry CV4 7AL, UK email: y.gomez@warwick.ac.uk
Francesca Faedi
Affiliation:
Department of Physics, University of Warwick, Coventry CV4 7AL, UK email: y.gomez@warwick.ac.uk
Leslie Hebb
Affiliation:
Department of Astronomy, University of Washington, Seattle, WA 98195, USA
Don Pollacco
Affiliation:
Department of Physics, University of Warwick, Coventry CV4 7AL, UK email: y.gomez@warwick.ac.uk
Keivan Stassun
Affiliation:
Department of Physics & Astronomy, Vanderbilt University, Nashville, TN 37235, USA
Phillip Cargile
Affiliation:
Department of Physics & Astronomy, Vanderbilt University, Nashville, TN 37235, USA
Barry Smalley
Affiliation:
Astrophysics Group, Keele University, Staffordshire ST5 5BG, UK
Amanda Doyle
Affiliation:
Astrophysics Group, Keele University, Staffordshire ST5 5BG, UK
Luan Ghezzi
Affiliation:
Observatório Nacional, Rua Gal. José Cristino 77, Rio de Janeiro, RJ 20921-400, Brazil
Susana C. C. Barros
Affiliation:
Laboratoire d'Astrophysique de Marseille UMR 7326, 13388, Marseille, France
Andrew Collier Cameron
Affiliation:
School of Physics and Astronomy, University of St Andrews, St Andrews, Fife KY16 9SS, UK
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Abstract

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The Homogeneous Study of Transiting Systems (HoSTS) will derive a consistent and homogeneous set of both the stellar and planetary physical properties for a large sample of bright transiting planetary systems with confirmed planetary masses and measured radii. Our resulting catalogs of the fundamental properties of these bright planets and their host stars will enable us to explore empirical correlations that will lead to a better understanding of planetary formation and evolution. We present our pilot study of the planet-hosting star WASP-13, and the framework of our project which will allow for the identification of true relationships among the physical properties of the systems from any systematics.

Keywords

stars: fundamental parametersplanetary systemstechniques: radial velocitiestechniques: spectroscopictechniques: techniques: photometricstars: individual (WASP-13)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 285 - 286
Copyright
Copyright © International Astronomical Union 2013 

References

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