  We present a new homogeneous survey of VLT/FLAMES LR8 line-of-sight radial
velocities (vlos) for 1604 resolved red giant branch stars in the Sculptor
dwarf spheroidal galaxy. In addition, we provide reliable Ca II triplet
metallicities, [Fe/H], for 1339 of these stars. From this combination of new
observations (2257 individual spectra) with ESO archival data (2389 spectra),
we obtain the largest and most complete sample of vlos and [Fe/H] measurements
for individual stars in any dwarf galaxy. Our sample includes VLT/FLAMES LR8
spectra for 55% of the red giant branch stars at G $<20$ from Gaia DR3, and
$>70$% of the brightest stars, G $<18.75$. Our spectroscopic velocities are
combined with Gaia DR3 proper motions and parallax measurements for a new and
more precise membership analysis. We look again at the global characteristics
of Sculptor, deriving a mean metallicity of $\langle$[Fe/H]$\rangle = -1.82 \pm
0.45$ and a mean line-of-sight velocity of $\langle$vlos$\rangle = +111.2 \pm
0.25$km/s. There is a clear metallicity gradient in Sculptor, -0.7deg/dex, with
the most metal-rich population being the most centrally concentrated.
Furthermore, the most metal-poor population in Sculptor, [Fe/H]$<-2.5$, appears
to show kinematic properties distinct from the rest of the stellar population.
Finally, we combine our results with the exquisite Gaia DR3 multi-colour
photometry to further investigate the colour-magnitude diagram of the resolved
stellar population in Sculptor. Our detailed analysis shows a similar global
picture as previous studies, but with much more precise detail, revealing that
Sculptor has more complex properties than previously thought. This survey
emphasises the role of the stellar spectroscopy technique and this galaxy as a
benchmark system for modelling galaxy formation and evolution on small scales.
