A High-precision Technique to Correct for Residual Atmospheric Dispersion in High-contrast Imaging Systems

A High-precision Technique to Correct for Residual Atmospheric Dispersion in High-contrast Imaging Systems

Direct detection and spectroscopy of exoplanets requires high-contrast imaging. For habitable exoplanets in particular, located at a small angular separation from the host star, it is crucial to employ small inner working angle (IWA) coronagraphs that efficiently suppress starlight. These coronagrap...

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Bibliographic Details
Main Authors: Pathak, P., Guyon, O., Jovanovic, N., Lozi, J., Martinache, F., Minowa, Y., Kudo, T., Takami, H., Hayano, Y., Narita, N.
Other Authors: Steward Observatory, University of Arizona
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
instrumentation: adaptive optics
atmospheric effects
planets and satellites: detection
Online Access:http://hdl.handle.net/10150/622414
http://arizona.openrepository.com/arizona/handle/10150/622414

Internet

http://hdl.handle.net/10150/622414
http://arizona.openrepository.com/arizona/handle/10150/622414

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