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Report by the ESA-ESO Working Group
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The working group membership was es
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3.2.2 The Darwin Ground-Based Precu
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Figure 1: Detection methods for ext
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those with masses between about 0.5
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Figure 2: Detection domains for met
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(c) Astrometric measurements do not
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Table 1: A summary of completed, op
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chemical composition of the primord
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Table 2: A summary of planned or op
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it passes behind the star. They arg
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shapes caused by extra-solar planet
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Table 3: A summary of completed, op
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ground requires simultaneous observ
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0.35 arcsec of the centre, i.e. muc
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ferential phase observations with a
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2.2 Space Observations: 2005-2015 I
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larger number of hot Jupiters would
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(Shao): this major SIM survey progr
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