172 citations · 1.6k across the 34 of their papers we have counts for
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astro-ph2005
Near-UV to near-IR disk-averaged Earth's spectra from Moon's Earthshine observations
S. Hamdani, L. Arnold, C. Foellmi +5
We discuss a series of Earthshine spectra obtained with the NTT/EMMI instrument between 320nm and 1020nm with a resolution of R~450 in the blue and R~250 in the red. These ascendin…
astro-ph2005★ 1 cited
On artificial transits feasibility and SETI
Luc Arnold
It is known that the shape of a planet (oblateness, rings, etc.) slightly modifies the shape of the transit light curve. The forthcoming space missions (Corot, Kepler), able to det…
astro-ph2005★ 92 cited
Transit Lightcurve Signatures of Artificial Objects
Luc Arnold
The forthcoming space missions, able to detect Earth-like planets by the transit method, will a fortiori also be able to detect the transit of artificial planet-size objects. Multi…