We should check at some point that we get the age distribution,
at a given metallicity, in the solar neighborhood (e.g. Schönrich & Binney)
right in the Stinson et al simulations.
Sonntag, 14. April 2013
Donnerstag, 11. April 2013
1st GES science meeting
Had some interesting conversations at the GES meeting:
-- immediate things to do:
* get access to the Edinburgh archive with Michelle and get the FGK stars out
* try to cross-match this with PS1 photometer
* distances should not come from only log_g; photometry has to come in.
-- mid-run:
* get best distances
* cross-correlate abundances GES-SDSS to get them at the same footing
* we need to get the best proper motions!!
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