Differences

This shows you the differences between two versions of the page.

--- gc5_program [2019/09/06 12:46] – added talk by T. Versic gmamon
+++ gc5_program [2022/10/24 11:57] (current) – external edit 127.0.0.1
@@ Line 7: / Line 7: @@
 |9:30      |//Gary Mamon//|Welcome|
 |9:40| //Gary Mamon//|Orbits of E, S, and S0 galaxies in clusters|
-|10:00| //Justin Read//| Dark matter heats up in dwarf galaxies|
+|10:00| //Klaudia Kowalczyk//|Applying multiple populations to Schwarzschild modelling|
-|10:20| //Klaudia Kowalczyk//|Applying multiple populations to Schwarzschild modelling|
+|10:20| //Eugene Vasiliev//|Distribution function-based modeling of mock and real dwarf spheroidals|
-|10:40| //Eugene Vasiliev//|Distribution function-based modeling of mock and real dwarf spheroidals|
+|10:40| //Anna Genina//| Simulated dwarfs in APOSTLE|
 |11:00| |COFFEE BREAK (Entrance Hall on ground floor) |
-|11:30| //Anna Genina//| Simulated dwarfs in APOSTLE|
+|11:30| //Justin Read//| Dark matter heats up in dwarf galaxies|
 |11:50| //Khyati Malhan//| Understanding the origin and morphology of the stellar streams as revealed by Gaia DR2|
-|12:10| //Nathaniel Starkman//| Extending the Pal5 Stream Detection Limits & Using Manifold Learning Techniques to Identify Stream Progenitors|
-|12:30| //Jason Sanders//| Measuring the Milky Way bar’s pattern speed using proper motion data and full 6D data|
 |12:50| |LUNCH|
 |14:45| | Analysis of mocks|
@@ Line 20: / Line 18: @@
 |16:45| | Analysis of mocks|
 |18:15| | END OF WORK DAY|
 ===== Tuesday: Salle des séminaires Evry Schatzman (basement) =====
 ^Time^Speaker^Topic^
-|9:30 |//Simon Rozier//|Linear stability of stellar rotating spheres|
+|9:30| //Nathaniel Starkman//| Extending the Pal5 Stream Detection Limits & Using Manifold Learning Techniques to Identify Stream Progenitors|
-|9:50 |//Tadeja Versic//|Observational requirements to resolve the core-cusp problem|
+|9:50| //Jason Sanders//| Measuring the Milky Way bar’s pattern speed using proper motion data and full 6D data|
-|10:10 |//Antonio Sollima//|Detection of the tidal tails of Galactic globular clusters using 5D mixture modelling|
+|10:10 |//Simon Rozier//|Linear stability of stellar rotating spheres|
-|10:30|//Farnik Nikakhtar//|New families in our solar neighborhood|
+|11:00| |COFFEE BREAK (Entrance Hall)|
-|11:00| | COFFEE BREAK (Entrance Hall)|
+|11:20 |//Tadeja Versic//|Observational requirements to resolve the core-cusp problem|
-|11:30| |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|
 |14:45| |Analysis of mocks|
@@ Line 35: / Line 33: @@
 |18:15| | END OF WORK DAY|
 ===== Wednesday: Salle des séminaires Evry Schatzman (basement) =====
-^Time^Topic^
+^Time^Speaker^Topic^
-|9:30 |Analysis of mocks|
+|9:30 |//Farnik Nikakhtar//|New families in our solar neighborhood|
-|11:00| COFFEE BREAK (Entrance Hall)|
+|9:50 | | Analysis of mocks|
-|11:30| Analysis of mocks|
+|11:00| | COFFEE BREAK (Entrance Hall)|
-|13:00| LUNCH|
+|11:30| | Analysis of mocks|
-|14:45| Analysis of mocks|
+|13:00| | LUNCH|
-|16:15| COFFEE BREAK (Entrance Hall)|
+|14:45| | Analysis of mocks|
-|16:45| Analysis of mocks|
+|16:15| | COFFEE BREAK (Entrance Hall)|
-|18:15| END OF WORK DAY|
+|16:45| | Analysis of mocks|
+|18:15| | END OF WORK DAY|
 ===== Thursday: Salle des séminaires Evry Schatzman (basement) =====
@@ Line 63: / Line 61: @@
 |11:00| COFFEE BREAK (Entrance Hall)|
 |11:30| Discussion and plans for future|
-|13:00| END OF MEETING|
+|12:45| END OF MEETING|
 [[gc5|Back to 5th Gaia Challenge workshop home page]]