The OAC-VST survey will be performed
in four bands. Two bands (V narrow and V) will cover a 64 square degree
field while the other two (R and z narrow) will cover only 1/6-th of the
field. The completion of the survey will require 56 night of OAC guaranteed
time distributed over three years.
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The limiting magnitudes are in the Vega system, integrated over a 3 arcsec circular aperture and at S/N=5. Limiting magnitudes for unresolved sources are ca. 1 mag fainter. Track for M* galaxies can be found here
Complementary photometry of the same field will be performed at CFH.
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