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Characterization of exoplanet atmospheres using future space-based infrared telescopes: challenges in detecting biomarkers

Published online by Cambridge University Press:  06 January 2014

Keigo Enya*
Affiliation:
Institute of Space and Astronautical Science, Japan Aerospace Exploration AgencyYoshinodai 3-1-1, Sagamihara, Kanagawa, Japan email: [email protected]
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Abstract

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Characterization of exoplanet atmospheres with space-based infrared telescopes is important to detect biomarkers. A promising method is temporary differential observation. For this method, designs of a wideband infrared spectral disperser are presented. A design using a CdTe prism simultaneously covers λ=1–30 μm. Designing binary pupil masks for segmented pupils to be used in spatially resolved observations are also shown for another observational method.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

Carlotti, A., Vanderbei, R., & Kasdin, N. J. 2011 arXiv:1108.4050Google Scholar
Doyon, R.et al. 2012, Proc. SPIE, 8442, 84422RGoogle Scholar
Enya, K. & Abe, L. 2010, PASJ, 62, 1407Google Scholar
Enya, K., Abe, L., Takeuchi, S., Kotani, T., & Yamamuro, T. 2011, Proc. SPIE, 8146, 81460QCrossRefGoogle Scholar
Enya, K. 2012, Proc. SPIE, 8442, 84423YCrossRefGoogle Scholar
Kopparapu, R. K., et al. 2013 ApJ, 765, 131Google Scholar
Vanderbei, R. J. 1999, Optimization methods and software, 11, 451Google Scholar