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The GROUnd-based Secondary Eclipse project - GROUSE

Published online by Cambridge University Press:  10 November 2011

Ernst de Mooij ,
Remco de Kok ,
Bas Nefs ,
Matteo Brogi  and
Ignas Snellen
Ernst de Mooij
Affiliation:
Leiden Observatory, Leiden University, Postbus 9513, 2300 RA, Leiden, The Netherlands; email: demooij@strw.leidenuniv.nl
Remco de Kok
Affiliation:
SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
Bas Nefs
Affiliation:
Leiden Observatory, Leiden University, Postbus 9513, 2300 RA, Leiden, The Netherlands; email: demooij@strw.leidenuniv.nl
Matteo Brogi
Affiliation:
Leiden Observatory, Leiden University, Postbus 9513, 2300 RA, Leiden, The Netherlands; email: demooij@strw.leidenuniv.nl
Ignas Snellen
Affiliation:
Leiden Observatory, Leiden University, Postbus 9513, 2300 RA, Leiden, The Netherlands; email: demooij@strw.leidenuniv.nl
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Abstract

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Secondary eclipse observations of exoplanets at near-infrared wavelengths are important to constrain the energy budgets of hot-Jupiters, since they probe the radiation from the planet's atmosphere at the peak of the spectral energy distribution. Since this wavelength range is accesible from the ground, we have started the GROUnd-based Secondary Eclipse (GROUSE) project. As part of the GROUSE project, we target a sample of hot-Jupiters at near-infrared and optical wavelengths. Planets include TrES-3b, HAT-P-1, WASP-18b and WASP-33b.

Keywords

techniques: photometricplanetary systems
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S276: The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution , October 2010 , pp. 487 - 488
Copyright
Copyright © International Astronomical Union 2011

References

Charbonneau, D., et al. 2005, ApJ, 626, 523CrossRefGoogle Scholar
Croll, B., Jayawardhana, R., Fortney, J. J., Lafrenire, D., & Albert, L. 2010, ApJ, 718, 920Google Scholar
Deming, D., Seager, S., Richardson, L. J., & Harrington, J. 2005, Nature, 434, 740CrossRefGoogle Scholar
De Mooij, E. J. W. & Snellen, I. A. G. 2009, A&A, 493, L35Google Scholar
De Mooij, E. J. W., De Kok, R. J., Nefs, S. V., & Snellen, I. A. G. 2011, A&A, 528, A49Google Scholar
Knutson, H. A., et al. 2008, ApJ, 673, 526CrossRefGoogle Scholar
Sing, D. K. & López-Morales, M. 2009, A&A, 493, L31Google Scholar