Feasibility of Earth-like planet detection with Extremely Large Telescopes
Abstract
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.
- Publication:
-
SF2A-2005: Semaine de l'Astrophysique Francaise
- Pub Date:
- December 2005
- Bibcode:
- 2005sf2a.conf..201B