  Prospects for future supernova surveys are discussed, focusing on the ESA
Euclid mission and the European Extremely Large Telescope(E-ELT), both expected
to be in operation around the turn of the decade. Euclid is a 1.2m space survey
telescope that will operate at visible and near-infrared wavelengths, and has
the potential to find and obtain multi-band lightcurves for thousands of
distant supernovae. The E-ELT is a planned general-purpose ground-based
40m-class optical-IR telescope with adaptive optics built in, which will be
capable of obtaining spectra of Type Ia supernovae to redshifts of at least
four. The contribution to supernova cosmology with these facilities will be
discussed in the context of other future supernova programs such as those
proposed for DES, JWST, LSST and WFIRST.
