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gc5_program [2019/09/09 17:23] – gmamongc5_program [2022/10/24 11:57] (current) – external edit 127.0.0.1
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 |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.1568049786.txt.gz · Last modified: 2022/10/24 11:56 (external edit)