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gc5_program [2019/09/09 17:23]
gmamon
gc5_program [2019/09/10 09:31] (current)
gmamon [Tuesday: Salle des séminaires Evry Schatzman (basement)]
Line 23: Line 23:
 |9:50| //Jason Sanders//| Measuring the Milky Way bar’s pattern speed using proper motion data and full 6D data| |9:50| //Jason Sanders//| Measuring the Milky Way bar’s pattern speed using proper motion data and full 6D data|
 |10:10 |//Simon Rozier//​|Linear stability of stellar rotating spheres| |10:10 |//Simon Rozier//​|Linear stability of stellar rotating spheres|
-|10:40 |//Tadeja Versic//​|Observational requirements to resolve the core-cusp problem| 
 |11:00| |COFFEE BREAK (Entrance Hall)| |11:00| |COFFEE BREAK (Entrance Hall)|
-|11:30 |//Antonio Sollima//​|Detection of the tidal tails of Galactic globular clusters using 5D mixture modelling| +|11:20 |//Tadeja Versic//​|Observational requirements to resolve the core-cusp problem| 
-|11:50| |Analysis of mocks|+|11:​40 ​|//Antonio Sollima//​|Detection of the tidal tails of Galactic globular clusters using 5D mixture modelling| 
 +|12:00| |Analysis of mocks|
 |13:00| | LUNCH| |13:00| | LUNCH|
 |14:45| |Analysis of mocks| |14:45| |Analysis of mocks|
gc5_program.txt · Last modified: 2019/09/10 09:31 by gmamon