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--- tests:collision:gc3 [2015/09/01 10:48] – gieles
+++ tests:collision:gc3 [2022/10/24 12:26] (current) – external edit 127.0.0.1
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 ===== GC III =====
+Active participants: Ian Claydon, Mark Gieles, Vincent Henault-Brunet, Miklos Peuten, Anna Lisa Varri, Laura Watkins, Alice Zocchi.
 ==== Goals/projects for GC III workshop ====
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   - Jeans modelling (Laura)
   - Single mass DF modelling (Alice)
-  - Multimass DF modelling (Miklos)
+  - Multimass DF modelling (Miklos, Mark)
+Results can go [[:tests:collision:gc3:method_comp|here]]
-The mock data is a snapshots of large $N$-body simulation of the globular cluster M4 are [[http://datashare.is.ed.ac.uk/handle/10283/618?show=full| available here]]. Full lists of data for all particles (mass, position, velocity, stellar type, stellar radius, V magnitude, B-V colour) are given at almost 400 instants in the lifetime of the model. The simulation is described in the [[http://arxiv.org/abs/1409.5597]], which should be cited when making use of this data.
-[[:tests:collision:gc3:method_comp|Jeans modelling vs. Distribution-function]] based models for fitting mock data of GCs.
-We will start with $N$-body snapshots of the M4 models by Heggie (2014): http://datashare.is.ed.ac.uk/handle/10283/618
 ===B. Understanding Gaia errors:===