Feasibility of Earth-like planet detection with Extremely Large Telescopes

Details Feasibility of Earth-like planet detection with Extremely Large Telescopes Feasibility of Earth-like planet detection with Extremely Large Telescopes

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..201b&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

This paper presents an attempt to compare the recent signal to noise
ratio calculations regarding the detection of Earth-like planets with
Extremely Large Telescopes. It is shown that although the models are
coherent, the hypothesis are different and lead to incompatible results
in terms of integration time.

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