Paper
14 July 2008 Spectral characterization of Earth-like transiting exoplanets
Wesley A. Traub, Lisa Kaltenegger, Kenneth W. Jucks
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Abstract
We calculate the expected signal-to-noise ratio (SNR) for spectral features in the transit spectrum of an Earth-like exoplanet, for the case of the nearest likely transit of a G and an M star, for a 6-m telescope in space. We find that the SNR values for all important spectral features, in the visible and infrared, are in the range 0.2 to 1.1, making the detection of such features difficult.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Wesley A. Traub, Lisa Kaltenegger, and Kenneth W. Jucks "Spectral characterization of Earth-like transiting exoplanets", Proc. SPIE 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 70101O (14 July 2008); https://doi.org/10.1117/12.788095
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Signal to noise ratio

Atmospheric modeling

Stars

Space telescopes

Earth's atmosphere

Planets

Infrared radiation

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