[x] What happens to hot stars? Check SPARV temperatures and include discussion (perhaps in context of odd projections of things outside of training set)
[x] Comment on the blue straggler mess --> they are all fast rotators, but their loggs are very slightly too low. Made more problematic by the fact they are fast rotating.
[x] Fix x-axis ranges of temperatures. Varies from (3500, 7500) to (4000, 8000)
[x] Sub-giant artefact --> comment on this
[x] Emphasize that the deltas in joining models are totally empirical (and give empirical justifications)
[x] Section 4.2.1 the calibration also uses Gaia benchmark stars, not just seismic information
[x] Figure 8: [M/H] in RAVE axes. Cull on: error in RV less than 8 km/s; c1 = c2 = c3 = n; TeffK > 4000 K
[x] Section 4.2.2. Figure 12, 13 appear before Figure 11
[x] Clarify with Steinmetz about individual giant/dwarf models available on request
[x] What is the S/N in the GES spectra that overlap with RAVE, and what fraction are UVES/GIRAFFE? Any unusual WG selection effects?
[x] Discuss origin of [Si/H] offset in RAVE/GES.
[x] GC section: 2 typos.
[x] OC section 4.3.2: stress that DR5 improves upon DR4
[x] De-scope DIBS and cite paper, put into discussion
Specifically:
Clarify with Steinmetz about individual giant/dwarf models available on request