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- W2012600482 abstract "There are good reasons for extending the spectral range of observation to shorter wavelengths than currently envisagedfor terrestrial planet-finding missions utilizing a 4-m, diffraction-limited, optical telescope. The angular resolution atshorter wavelengths is higher, so that the image of an exoplanet is better separated from that of the much brighter star.Due to the higher resolution, the exozodiacal background per resolution element is smaller, so exposure times arereduced for the same incident flux. Most importantly, the sensitivity to the presence of life on habitable exoplanets isincreased over a hundred-fold by access to the ozone biomarker in the mid-ultraviolet. These benefits must be weighedagainst challenges arising from the faintness of exoplanets in the mid-UV. Here, we describe the benefits, technicalchallenges and some proposed solutions for detecting ozone in the atmospheres of Earth-like exoplanets." @default.
- W2012600482 created "2016-06-24" @default.
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- W2012600482 date "2008-07-12" @default.
- W2012600482 modified "2023-09-23" @default.
- W2012600482 title "Detecting biomarkers in exoplanetary atmospheres with a Terrestrial Planet Finder" @default.
- W2012600482 doi "https://doi.org/10.1117/12.787141" @default.
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