22 April 2008 Exoplanets: Which wavelengths?
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Proceedings Volume 6986, Extremely Large Telescopes: Which Wavelengths? Retirement Symposium for Arne Ardeberg; 69860B (2008) https://doi.org/10.1117/12.801262
Event: Extremely Large Telescopes: Which Wavelengths? Retirement Symposium for Arne Ardeberg, 2007, Lund, Sweden
Abstract
The physical basis of the detection and characterisation of extrasolar Earth-like planets and of biosignatures in the reflected light and thermal emission regimes is reviewed. Both approaches have their advantages and disadvantages, including artefacts, in the determination of planet physical parameters (mass, size, albedo, surface and atmospheric conditions etc) and biosignatures.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. Schneider, J. Schneider, } "Exoplanets: Which wavelengths?", Proc. SPIE 6986, Extremely Large Telescopes: Which Wavelengths? Retirement Symposium for Arne Ardeberg, 69860B (22 April 2008); doi: 10.1117/12.801262; https://doi.org/10.1117/12.801262
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