  The Supernova Cosmology Project has conducted the `See Change' programme,
aimed at discovering and observing high-redshift (1.13 $\leq$ z $\leq$ 1.75)
Type Ia supernovae (SNe Ia). We used multi-filter Hubble Space Telescope (HST)
observations of massive galaxy clusters with sufficient cadence to make the
observed SN Ia light curves suitable for a cosmological probe of dark energy at
z > 0.5. This See Change sample of SNe Ia with multi-colour light curves will
be the largest to date at these redshifts. As part of the See Change programme,
we obtained ground-based spectroscopy of each discovered transient and/or its
host galaxy. Here we present Very Large Telescope (VLT) spectra of See Change
transient host galaxies, deriving their redshifts, and host parameters such as
stellar mass and star formation rate. Of the 39 See Change transients/hosts
that were observed with the VLT, we successfully determined the redshift for
26, including 15 SNe Ia at z > 0.97. We show that even in passive environments,
it is possible to recover secure redshifts for the majority of SN hosts out to
z = 1.5. We find that with typical exposure times of 3 - 4 hrs on an 8m-class
telescope we can recover ~75% of SN Ia redshifts in the range of 0.97 < z <
1.5. Furthermore, we show that the combination of HST photometry and VLT
spectroscopy is able to provide estimates of host galaxy stellar mass that are
sufficiently accurate for use in a mass-step correction in the cosmological
analysis.
