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Searching for Faint Exozodiacal Disks: Keck Results and LBTI Status

Published online by Cambridge University Press:  06 January 2014

D. Defrère
Affiliation:
Steward Observatory email: [email protected]
P. Hinz
Affiliation:
Steward Observatory email: [email protected]
B. Mennesson
Affiliation:
Jet Propulsion Laboratory
R. Millan-Gabet
Affiliation:
Caltech
A. Skemer
Affiliation:
Steward Observatory email: [email protected]
V. Bailey
Affiliation:
Steward Observatory email: [email protected]
T.J. Rodigas
Affiliation:
Steward Observatory email: [email protected]
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Abstract

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The possible presence of dust in the habitable zone around nearby main-sequence stars is considered as a major hurdle toward the direct imaging of Earth-like extrasolar planets with future dedicated space-based telescopes (e.g., Roberge et al. 2012). In this context, NASA has funded two ground-based mid-infrared nulling interferometers to combine the large apertures available at the Keck Observatory and the Large Binocular Telescope (LBT). In this poster, we present the preliminary results of the extended survey carried out with the Keck Interferometer Nuller (KIN) between 2008 and 2011 and describe the forthcoming LBTI survey.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

Absil, O., et al., 2013, A&A, 555, 104Google Scholar
Bracewell, R. N., 1978, Nature, 274, 780.CrossRefGoogle Scholar
Martin, S., et al., 2012, AO 51 39073921.Google Scholar
Mennesson, B., et al., 2011, ApJ, 243, 178.CrossRefGoogle Scholar
Millan-Gabet, R., et al., 2011, ApJ, 734, 67.CrossRefGoogle Scholar
Roberge, A., et al., 2012, PASP 124 799808.CrossRefGoogle Scholar
Stock, N. D., et al., 2010, ApJ 724 12381255.CrossRefGoogle Scholar