  We analyse the detectability of vegetation on a global scale on Earth's
surface. Considering its specific reflectance spectrum showing a sharp edge
around 700 nm, vegetation can be considered as a potential global biomarker.
This work, based on observational data, aims to characterise and to quantify
this signature in the disk-averaged Earth's spectrum. Earthshine spectra have
been used to test the detectability of the "Vegetation Red Edge" (VRE) in the
Earth spectrum. We obtained reflectance spectra from near UV (320 nm) to near
IR (1020 nm) for different Earth phases (continents or oceans seen from the
Moon) with EMMI on the NTT at ESO/La Silla, Chile. We accurately correct the
sky background and take into account the phase-dependent colour of the Moon.
VRE measurements require a correction of the ozone Chappuis absorption band and
Rayleigh plus aerosol scattering. Results : The near-UV spectrum shows a dark
Earth below 350 nm due to the ozone absorption. The Vegetation Red Edge is
observed when forests are present (4.0% for Africa and Europe), and is lower
when clouds and oceans are mainly visible (1.3% for the Pacific Ocean). Errors
are typically $\pm0.5$, and $\pm1.5$ in the worst case. We discuss the
different sources of errors and bias and suggest possible improvements. We
showed that measuring the VRE or an analog on an Earth-like planet remains very
difficult (photometric relative accuracy of 1% or better). It remains a small
feature compared to atmospheric absorption lines. A direct monitoring from
space of the global (disk-averaged) Earth's spectrum would provide the best VRE
follow-up.
