Spectral Image Models of Planetary Systems for Simulating Exoplanet Observations
Future missions to characterize exoplanets will require instruments tailored to finding a habitable exoplanet: suppressing the bright star while still directly observing planets at small angular separations. This problem is compounded by interplanetary dust, a significant source of astrophysical bac...
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| Language: | en_US |
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The University of Arizona.
2015
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| Online Access: | http://hdl.handle.net/10150/579279 |