Make the following checks and figures from the RAVE/Cannon results:
[x] LOOCV on the training set
[x] Comparison to DR4 stellar parameters
[X] Comparison to literature studies (as per Kordopatis+ 14)
[x] Identify repeat observations and plot label precision as a function of S/N
[x] Comparison with GES overlap
[x] Comparison with K2 EPIC (Huber+ 2016; 4611 matches) (LOOCV will suffice)
[x] Cross-match against public catalogs of nu_max and compare seismic logg values (None exist!)
[x] Identify open clusters and look at their metallicity distributions (for homogeneity/precision) [@keithhawkins tasked]
[x] Identify globular clusters and verify that we see the general abundance trends as reported in the literature [@keithhawkins tasked]
[x] Show one-to-one labels and differences with "gold standards": Reddy (2003, 2006), V & F (2005), Bensby (2014)
[x] Make a HRD compared to "gold standards" in other panels: (a): our work with SNR>50 or something, (b): Reddy (2003, 2006), (c): Valenti & Fishcer (2005), (d): Bensby+ (2014)
[x] Compare abundances with Reddy, V + F, Bensby --> (Out of scope until main-sequence abundances exist)
Make the following checks and figures from the RAVE/Cannon results:
Comparison with K2 EPIC (Huber+ 2016; 4611 matches)(LOOCV will suffice)Cross-match against public catalogs of nu_max and compare seismic logg values(None exist!)Compare abundances with Reddy, V + F, Bensby--> (Out of scope until main-sequence abundances exist)