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Exoplanet transit spectro-photometry with SOFIA

Published online by Cambridge University Press:  10 November 2011

Daniel Angerhausen
Affiliation:
Deutsches SOFIA Institut, Universität Stuttgart, Pfaffenwaldring 31, 70569 Stuttgart, Germany email: angerhausen@irs.uni-stuttgart.de
Alfred Krabbe
Affiliation:
Deutsches SOFIA Institut, Universität Stuttgart, Pfaffenwaldring 31, 70569 Stuttgart, Germany email: angerhausen@irs.uni-stuttgart.de
Hans Zinnecker
Affiliation:
Deutsches SOFIA Institut, Universität Stuttgart, Pfaffenwaldring 31, 70569 Stuttgart, Germany email: angerhausen@irs.uni-stuttgart.de
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Abstract

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We present the prospects of observing extrasolar planets with the Stratospheric Observatory for Infrared Astronomy (SOFIA). Our analysis shows that optical and near-infrared photometric and spectrophotometric follow-up observations during planetary transits and\break eclipses will be feasible with SOFIA's instrumentation, especially with the HIPO-FLITECAM optical/NIR instruments. SOFIA has unique advantages in comparison to ground- and space-based observatories in this field of research which will be outlined.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Angerhausen, D., Krabbe, A., & Iserlohe, C. 2010, PASP, 122, 1020CrossRefGoogle Scholar
Gehrz, R. D., Becklin, E. E., de Pater, I., Lester, D. F., Roellig, T. L., & Woodward, C. E. 2009, AdSR, 44, 413Google Scholar
Swain, M. R., et al. 2009, ApJ, 704, 1616CrossRefGoogle Scholar